Le rôle du récepteur scavenger B type I, SR-BI, dans l'absorption et le métabolisme du cholestérol au niveau intestinal

Mémoire numérisé par la Direction des bibliothèques de l'Université de Montréal.

Le rôle du récepteur scavenger B type I, SR-BI, dans l'absorption et le métabolisme du cholestérol au niveau intestinal

Mémoire numérisé par la Direction des bibliothèques de l'Université de Montréal.

The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars

How do the magnetic fields of massive stars evolve over time? Are their gyrochronological ages consistent with ages inferred from evolutionary tracks? Why do most stars predicted to host Centrifugal Magnetospheres (CMs) display no H$\alpha$ emission? Does plasma escape from CMs via centrifugal breakout events, or by a steady-state leakage mechanism? This thesis investigates these questions via a population study with a sample of 51 magnetic early B-type stars. The longitudinal magnetic field \bz~was measured from Least Squares Deconvolution profiles extracted from high-resolution spectropolarimetric data. New rotational periods $P_{\rm rot}$ were determined for 15 stars from \bz, leaving only 3 stars for which $P_{\rm rot}$ is unknown. Projected rotational velocities \vsini~were measured from multiple spectral lines. Effective temperatures and surface gravities were measured via ionization balances and line profile fitting of H Balmer lines. Fundamental physical parameters, \bz, \vsini, and $P_{\rm rot}$ were then used to determine radii, masses, ages, dipole oblique rotator model, stellar wind, magnetospheric, and spindown parameters using a Monte Carlo approach that self-consistently calculates all parameters while accounting for all available constraints on stellar properties. Dipole magnetic field strengths $B_{\rm d}$ follow a log-normal distribution similar to that of Ap stars, and decline over time in a fashion consistent with the expected conservation of fossil magnetic flux. $P_{\rm rot}$ increases with fractional main sequence age, mass, and $B_{\rm d}$, as expected from magnetospheric braking. However, comparison of evolutionary track ages to maximum spindown ages $t_{\rm S,max}$ shows that initial rotation fractions may be far below critical for stars with $M_*>10 M_\odot$. Computing $t_{\rm S,max}$ with different mass-loss prescriptions indicates that the mass-loss rates of B-type stars are likely much lower than expected from extrapolation from O-type stars. Stars with H$\alpha$ in emission and absorption occupy distinct regions in the updated rotation-magnetic confinement diagram: H$\alpha$-bright stars are found to be younger, more rapidly rotating, and more strongly magnetized than the general population. Emission strength is sensitive both to the volume of the CM and to the mass-loss rate, favouring leakage over centrifugal breakout.

Cost-effectiveness of natriuretic peptide-based screening and collaborative care: a report from the STOP-HF (St Vincent's Screening TO Prevent Heart Failure) study

AIMS: Prevention of cardiovascular disease and heart failure (HF) in a cost-effective manner is a public health goal. This work aims to assess the cost-effectiveness of the St Vincent's Screening TO Prevent Heart Failure (STOP-HF) intervention.

METHODS AND RESULTS: This is a substudy of 1054 participants with cardiovascular risk factors [median age 65.8 years, interquartile range (IQR) 57.8:72.4, with 4.3 years, IQR 3.4:5.2, follow-up]. Annual natriuretic peptide-based screening was performed, with collaborative cardiovascular care between specialist physicians and general practitioners provided to patients with BNP levels >50 pg/mL. Analysis of cost per case prevented and cost-effectiveness per quality-adjusted life year (QALY) gained was performed. The primary clinical endpoint of LV dysfunction (LVD) with or without HF was reduced in intervention patients [odds ratio (OR) 0.60; 95% confidence interval (CI) 0.38-0.94; P = 0.026]. There were 157 deaths and/or emergency hospitalizations for major adverse cardiac events (MACE) in the control group vs. 102 in the intervention group (OR 0.68; 95% CI 0.49-0.93; P = 0.01). The cost per case of LVD/HF prevented was €9683 (sensitivity range -€843 to €20 210), whereas the cost per MACE prevented was €3471 (sensitivity range -€302 to €7245). Cardiovascular hospitalization savings offset increased outpatient and primary care costs. The cost per QALY gain was €1104 and the intervention has an 88% probability of being cost-effective at a willingness to pay threshold of €30 000.

CONCLUSION: Among patients with cardiovascular risk factors, natriuretic peptide-based screening and collaborative care reduced LVD, HF, and MACE, and has a high probability of being cost-effective.

TRIAL REGISTRATION: NCT00921960.

The VLT-FLAMES Tarantula Survey: XIX. B-type supergiants: Atmospheric parameters and nitrogen abundances to investigate the role of binarity and the width of the main sequence

Context: Model atmosphere analyses have been previously undertaken for both Galactic and extragalactic B-type supergiants. By contrast, little attention has been given to a comparison of the properties of single supergiants and those that are members of multiple systems. 

Aims: Atmospheric parameters and nitrogen abundances have been estimated for all the B-type supergiants identified in the VLT-FLAMES Tarantula survey. These include both single targets and binary candidates. The results have been analysed to investigate the role of binarity in the evolutionary history of supergiants. 

Methods: tlusty non-local thermodynamic equilibrium (LTE) model atmosphere calculations have been used to determine atmospheric parameters and nitrogen abundances for 34 single and 18 binary supergiants. Effective temperatures were deduced using the silicon balance technique, complemented by the helium ionisation in the hotter spectra. Surface gravities were estimated using Balmer line profiles and microturbulent velocities deduced using the silicon spectrum. Nitrogen abundances or upper limits were estimated from the Nii spectrum. The effects of a flux contribution from an unseen secondary were considered for the binary sample. Results. We present the first systematic study of the incidence of binarity for a sample of B-type supergiants across the theoretical terminal age main sequence (TAMS). To account for the distribution of effective temperatures of the B-type supergiants it may be necessary to extend the TAMS to lower temperatures. This is also consistent with the derived distribution of mass discrepancies, projected rotational velocities and nitrogen abundances, provided that stars cooler than this temperature are post-red supergiant objects. For all the supergiants in the Tarantula and in a previous FLAMES survey, the majority have small projected rotational velocities. The distribution peaks at about 50 km s^-1 with 65% in the range 30 km s^-1 ≤ ν_e sin i ≤ 60 km s^-1. About ten per cent have larger ve sin i (≥100 km s^-1), but surprisingly these show little or no nitrogen enhancement. All the cooler supergiants have low projected rotational velocities of ≤70 km s^-1 and high nitrogen abundance estimates, implying that either bi-stability braking or evolution on a blue loop may be important. Additionally, there is a lack of cooler binaries, possibly reflecting the small sample sizes. Single-star evolutionary models, which include rotation, can account for all of the nitrogen enhancement in both the single and binary samples. The detailed distribution of nitrogen abundances in the single and binary samples may be different, possibly reflecting differences in their evolutionary history. 

Conclusions: The first comparative study of single and binary B-type supergiants has revealed that the main sequence may be significantly wider than previously assumed, extending to T_eff = 20 000 K. Some marginal differences in single and binary atmospheric parameters and abundances have been identified, possibly implying non-standard evolution for some of the sample. This sample as a whole has implications for several aspects of our understanding of the evolutionary status of blue supergiants.

The VLT-FLAMES Tarantula Survey: XVIII. Classifications and radial velocities of the B-type stars

We present spectral classifications for 438 B-type stars observed as part of the VLT-FLAMES Tarantula Survey (VFTS) in the 30 Doradus region of the Large Magellanic Cloud. Radial velocities are provided for 307 apparently single stars, and for 99 targets with radial-velocity variations which are consistent with them being spectroscopic binaries. We investigate the spatial distribution of the radial velocities across the 30 Dor region, and use the results to identify candidate runaway stars. Excluding potential runaways and members of two older clusters in the survey region (SL 639 and Hodge 301), we determine a systemic velocity for 30 Dor of 271.6 ± 12.2 km s^-1 from 273 presumed single stars. Employing a 3σ criterion we identify nine candidate runaway stars (2.9% of the single stars with radial-velocity estimates). The projected rotational velocities of the candidate runaways appear to be significantly different to those of the full B-type sample, with a strong preference for either large (≥345 km s^-1) or small (≤65 km s^-1) rotational velocities. Of the candidate runaways, VFTS 358 (classified B0.5: V) has the largest differential radial velocity (-106.9 ± 16.2 km s^-1), and a preliminary atmospheric analysis finds a significantly enriched nitrogen abundance of 12 + log (N/H) ≳ 8.5. Combined with a large rotational velocity (υ_e sin i = 345 ± 22 km s^-1), this is suggestive of past binary interaction for this star.

The VLT-FLAMES tarantula survey:X. Evidence for a bimodal distribution of rotational velocities for the single early B-type stars

Aims. Projected rotational velocities (ve sin i) have been estimated for 334 targets in the VLT-FLAMES Tarantula Survey that do not manifest significant radial velocity variations and are not supergiants. They have spectral types from approximately O9.5 to B3. The estimates have been analysed to infer the underlying rotational velocity distribution, which is critical for understanding the evolution of massive stars. Methods. Projected rotational velocities were deduced from the Fourier transforms of spectral lines, with upper limits also being obtained from profile fitting. For the narrower lined stars, metal and non-diffuse helium lines were adopted, and for the broader lined stars, both non-diffuse and diffuse helium lines; the estimates obtained using the different sets of lines are in good agreement. The uncertainty in the mean estimates is typically 4% for most targets. The iterative deconvolution procedure of Lucy has been used to deduce the probability density distribution of the rotational velocities. Results. Projected rotational velocities range up to approximately 450 kms-1 and show a bi-modal structure. This is also present in the inferred rotational velocity distribution with 25% of the sample having 0 <ve <100 km s^-1 and the high velocity component having v_e ∼ 250 km s^-1. There is no evidence from the spatial and radial velocity distributions of the two components that they represent either field and cluster populations or different episodes of star formation. Be-type stars have also been identified. Conclusions. The bi-modal rotational velocity distribution in our sample resembles that found for late-B and early-A type stars.While magnetic braking appears to be a possible mechanism for producing the low-velocity component, we can not rule out alternative explanations. © ESO 2013.

A Rare Loss-of-Function Variant in Scavenger Receptor Class B Type I (SCARB1) Raises HDL Cholesterol and Increases Risk of Coronary Disease

Scavenger receptor BI (SR-BI) is the major receptor for high-density lipoprotein (HDL)
cholesterol (HDL-C). In humans, high amounts of HDL-C in plasma are associated with a
lower risk of coronary heart disease (CHD). Mice that have depleted Scarb1 (SR-BI
knockout mice) have markedly elevated HDL-C levels but, paradoxically, increased
atherosclerosis. The impact of SR-BI on HDL metabolism and CHD risk in humans remains
unclear. Through targeted sequencing of coding regions of lipid-modifying genes in 328
individuals with extremely high plasma HDL-C levels, we identified a homozygote for a lossof-function
variant, in which leucine replaces proline 376 (P376L), in SCARB1, the gene
encoding SR-BI. The P376L variant impairs posttranslational processing of SR-BI and
abrogates selective HDL cholesterol uptake in transfected cells, in hepatocyte-like cells
derived from induced pluripotent stem cells from the homozygous subject, and in mice.
Large population-based studies revealed that subjects who are heterozygous carriers of
the P376L variant have significantly increased levels of plasma HDL-C. P376L carriers have
a profound HDL-related phenotype and an increased risk of CHD (odds ratio = 1.79, which is
statistically significant).

Advanced chronic heart failure: A position statement from the Study Group on Advanced Heart Failure of the Heart Failure Association of the European Society of Cardiology

Therapy has improved the survival of heart failure (HF) patients. However, many patients progress to advanced chronic HF (ACHF). We propose a practical clinical definition and describe the characteristics of this condition. Patients that are generally recognised as ACHF often exhibit the following characteristics: 1) severe symptoms (NYHA class III to IV); 2) episodes with clinical signs of fluid retention and/or peripheral hypoperfusion; 3) objective evidence of severe cardiac dysfunction, shown by at least one of the following: left ventricular ejection fraction<30%, pseudonormal or restrictive mitral inflow pattern at Doppler-echocardiography; high left and/or right ventricular filling pressures; elevated B-type natriuretic peptides; 4) severe impairment of functional capacity demonstrated by either inability to exercise, a 6-minute walk test distance<300 m or a peak oxygen uptake<12-14 ml/kg/min; 5) history of >1 HF hospitalisation in the past 6 months; 6) presence of all the previous features despite optimal therapy. This definition identifies a group of patients with compromised quality of life, poor prognosis, and a high risk of clinical events. These patients deserve effective therapeutic options and should be potential targets for future clinical research initiatives.

Spatiotemporal dynamics of guanosine 3′,5′-cyclic monophosphate revealed by a genetically encoded, fluorescent indicator

To investigate the dynamics of guanosine 3′,5′-cyclic monophosphate (cGMP) in single living cells, we constructed genetically encoded, fluorescent cGMP indicators by bracketing cGMP-dependent protein kinase (cGPK), minus residues 1–77, between cyan and yellow mutants of green fluorescent protein. cGMP decreased fluorescence resonance energy transfer (FRET) and increased the ratio of cyan to yellow emissions by up to 1.5-fold with apparent dissociation constants of ≈2 μM and >100:1 selectivity for cGMP over cAMP. To eliminate constitutive kinase activity, Thr516 of cGPK was mutated to Ala. Emission ratio imaging of the indicators transfected into rat fetal lung fibroblast (RFL)-6 showed cGMP transients resulting from activation of soluble and particulate guanylyl cyclase, respectively, by nitric oxide (NO) and C-type natriuretic peptide (CNP). Whereas all naive cells tested responded to CNP, only 68% responded to NO. Both sets of signals showed large and variable (0.5–4 min) latencies. The phosphodiesterase (PDE) inhibitor 3-isobutyl-1-methylxanthine (IBMX) did not elevate cGMP on its own but consistently amplified responses to NO or CNP, suggesting that basal activity of guanylate cyclase is very low and emphasizing the importance of PDEs in cGMP recycling. A fraction of RFL cells showed slowly propagating tides of cGMP spreading across the cell in response to delocalized application of NO. Biolistically transfected Purkinje neurons showed cGMP responses to parallel fiber activity and NO donors, confirming that single-cell increases in cGMP occur under conditions appropriate to cause synaptic plasticity.

Late cardiac effects of chemotherapy in breast cancer survivors treated with adjuvant doxorubicin: 10-year follow-up

Doxorubicin (Dox), a mainstay of adjuvant breast cancer treatment, is associated with cardiac toxicity in the form of left ventricular dysfunction (LVD), LV diastolic dysfunction, or LV systolic dysfunction. Study objectives were to evaluate the prevalence of LVD in long-term breast cancer survivors treated with Dox and determine if brain-type natriuretic peptide (BNP) may help identify patients at risk for LVD. Patients who participated in prospective clinical trials of adjuvant Dox-based chemotherapy for breast cancer with a baseline left ventricular (LV) ejection fraction evaluation from 1999 to 2006 were retrospectively identified from the St Vincent's University Hospital database. Patients were invited to undergo transthoracic echocardiography, BNP analysis, and cardiovascular (CV) risk factor assessment. LVDD was defined as left atrial volume index >34 mL/m(2) and/or lateral wall E prime <10 m/s, and LVSD as LVEF <50 %. Of 212 patients identified, 154 participated, 19 patients had died (no cardiac deaths), and 39 declined. Mean age was 60.7 [55:67] years. A majority of the patients (128, 83 %) had low CV risk (0/1 risk factors), 21 (13.6 %) had 2 RFs, and 5 (3.2 %) ≥3 RFs. BMI was 27.2 ± 4.9 kg/m(2). Median Dox dose was 240 mg/m(2) [225-298]; 92 patients (59.7 %) received ≤240 mg/m(2) and 62 (40.3 %) > 240 mg/m(2). Baseline LVEF was 68.2 ± 8 %. At follow-up of 10.8 ± 2.2 years, LVEF was 64.4 ± 6 %. Three (1.9 %) subjects had LVEF <50 % and one (0.7 %) had LVDD. Dox >240 mg/m2 was associated with any LVEF drop. BNP levels at follow-up were 20.3 pg/ml [9.9-36.5] and 21.1 pg/ml [9.8-37.7] in those without LVD and 61.5 pg/ml [50-68.4] in those with LVD (p = 0.04). Long-term prospective data describing the impact of Dox on cardiotoxicity are sparse. At over 10 years of follow-up, decreases in LVEF are common, and dose related, but LVD as defined is infrequent (2.6 %). Monitoring with BNP for subclinical LVD needs further evaluation.

The T-381C SNP in BNP gene may be modestly associated with type 2 diabetes: an updated meta-analysis in 49 279 subjects.

A recent study reported an association between the brain natriuretic peptide (BNP) promoter T-381C polymorphism (rs198389) and protection against type 2 diabetes (T2D). As replication in several studies is mandatory to confirm genetic results, we analyzed the T-381C polymorphism in seven independent case-control cohorts and in 291 T2D-enriched pedigrees totalling 39 557 subjects of European origin. A meta-analysis of the seven case-control studies (n = 39 040) showed a nominal protective effect [odds ratio (OR) = 0.86 (0.79-0.94), P = 0.0006] of the CC genotype on T2D risk, consistent with the previous study. By combining all available data (n = 49 279), we further confirmed a modest contribution of the BNP T-381C polymorphism for protection against T2D [OR = 0.86 (0.80-0.92), P = 1.4 x 10(-5)]. Potential confounders such as gender, age, obesity status or family history were tested in 4335 T2D and 4179 normoglycemic subjects and they had no influence on T2D risk. This study provides further evidence of a modest contribution of the BNP T-381C polymorphism in protection against T2D and illustrates the difficulty of unambiguously proving modest-sized associations even with large sample sizes.

Le peptide natriurétique auriculaire induit la différenciation cardiaque dans les cellules souches embryonnaires carcinomateuses de souris P19

Traditionnellement associée à la reproduction féminine, l'ocytocine (OT), une hormone peptidique synthétisée par les noyaux paraventriculaire et supraoptique de l'hypothalamus et sécrétée par l'hypophyse postérieure (neurohypophyse), a été récemment revue et a été démontrée avoir plusieurs nouveaux rôles dans le système cardio-vasculaire. En effet, notre laboratoire a montré que l’OT peut induire la différenciation des cellules souches embryonnaires (CSE) en cardiomyocytes (CM) fonctionnels. À l’aide du modèle cellulaire embryonnaire carcinomateux de souris P19, il a été démontré que ce processus survenait suite à la libération de la guanosine monophosphate cyclique (GMPc) dépendante du monoxyde d’azote. De même, il est connu que le peptide natriurétique auriculaire (ANP), un peptide produit, stocké et sécrété par les myocytes cardiaques, peut aussi induire la production du GMPc. De nombreuses études ont démontré que le cœur ayant subi un infarctus pouvait être régénéré à partir d’une population isolée de cellules souches et progénitrices transplantées. Une de ces populations de cellules, fréquemment isolées à partir d'organes provenant d'animaux aux stades de développement embryonnaire et adulte, appelée « Side Population » (SP), sont identifiées par cytométrie en flux (FACS) comme une population de cellules non marquées par le colorant fluorescent Hoechst 33342 (Ho). Les cellules SP expriment des protéines de transport spécifiques, de la famille ATP-binding cassette, qui ont pour rôle de transporter activement le colorant fluorescent Ho de leur cytoplasme. La sous-population de cellules SP isolée du cœur affiche un potentiel de différenciation cardiaque amélioré en réponse à un traitement avec l’OT. Récemment, l'hétérogénéité phénotypique et fonctionnelle des CSE a été mise en évidence, et cela a été corrélé avec la présence de sous-populations cellulaires ressemblant beaucoup aux cellules SP issues du cœur. Puisque l’ANP peut induire la production du GMPc et qu’il a été démontré que la différenciation cardiaque était médiée par la production du GMPc, alors nous émettons l'hypothèse selon laquelle l’ANP pourrait induire la différenciation cardiaque. Étant donné que les CSE sont composés d’un mélange de différents types cellulaires alors nous émettons aussi l’hypothèse selon laquelle l’utilisation d’une sous-population de CSE plus homogène renforcerait le potentiel de différenciation de l'ANP. Méthodes : Les SP ont été isolées des cellules P19 par FACS en utilisant la méthode d’exclusion du colorant fluorescent Ho. Puis, leur phénotype a été caractérisé par immunofluorescence (IF) pour les marqueurs de l’état indifférencié, d’auto-renouvellement et de pluripotence octamer-binding transcription factor 4 (OCT4) et stage-specific embryonic antigen-1 (SSEA1). Ensuite, la dose pharmacologique optimale d’ANP a été déterminée via des tests de cytotoxicité sur des cellules P19 (MTT assay). Pour induire la différenciation en cardiomyocytes, des cellules à l’état de sphéroïdes ont été formées à l’aide de la technique du « Hanging-Drop » sous la stimulation de l’ANP pendant 5 jours. Puis, des cryosections ont été faites dans les sphéroïdes afin de mettre en évidence la présence de marqueurs de cellules cardiaques progénitrices tels que GATA4, Nkx2.5 et un marqueur mitochondrial spécifique Tom22. Ensuite, les cellules SP P19 ont été stimulées dans les sphéroïdes cellulaires par le traitement avec de l'ANP (10-7 M) ou de l’OT (10-7 M), de l’antagoniste spécifique du guanylate cyclase particulé (GCp) A71915 (10-6 M), ainsi que la combinaison des inducteurs OT+ANP, OT+A71915, ANP+A71915. Après la mise en culture, la différenciation en cardiomyocytes a été identifié par l’apparition de colonies de cellules battantes caractéristiques des cellules cardiaques, par la détermination du phénotype cellulaire par IF, et enfin par l’extraction d'ARN et de protéines qui ont été utilisés pour le dosage du GMPc par RIA, l’expression des ARNm par RT-PCR et l’expression des protéines par immunobuvardage de type western. Résultats : Les sphéroïdes obtenus à l’aide de la technique du « Hanging-Drop » ont montré une hausse modeste de l’expression des ARNm suivants : OTR, ANP et GATA4 comparativement aux cellules cultivées en monocouches. Les sphéroïdes induits par l’ANP ont présenté une augmentation significative des facteurs de transcription cardiaque GATA4 et Nkx2.5 ainsi qu’un plus grand nombre de mitochondries caractérisé par une plus grande présence de Tom22. De plus, L’ANP a induit l’apparition de colonies de cellules battantes du jour 7 (stade précoce) au jour 14 (stade mature) de façon presque similaire à l’OT. Cependant, la combinaison de l’ANP avec l’OT n’a pas induit de colonies de cellules battantes suggérant un effet opposé à celui de l’OT. Par IF, nous avons quantifié (nombre de cellules positives) et caractérisé, du jour 6 au jour 14 de différenciation, le phénotype cardiaque de nos cellules en utilisant les marqueurs suivants : Troponine T Cardiaque, ANP, Connexines 40 et 43, l’isoforme ventriculaire de la chaîne légère de myosine (MLC-2v), OTR. Les SP différenciées sous la stimulation de l’ANP ont montré une augmentation significative du GMPc intracellulaire comparé aux cellules non différenciées. À notre grande surprise, l’antagoniste A71915 a induit une plus grande apparition de colonies de cellules battantes comparativement à l’OT et l’ANP à un jour précoce de différenciation cardiaque et l’ajout de l’OT ou de l’ANP a potentialisé ses effets, augmentant encore plus la proportion de colonies de cellules battantes. De plus, la taille des colonies de cellules battantes était encore plus importante que sous la simple stimulation de l’OT ou de l’ANP. Les analyses radioimmunologiques dans les cellules SP P19 stimulés avec l’ANP, A71915 et la combinaison des deux pendant 15min, 30min et 60min a montré que l’ANP stimule significativement la production du GMPc, cependant A71915 n’abolit pas les effets de l’ANP et celui-ci au contraire stimule la production du GMPc via des effets agonistes partiels. Conclusion : Nos résultats démontrent d’une part que l’ANP induit la différenciation des cellules SP P19 en CM fonctionnels. D’autre part, il semblerait que la voie de signalisation NPRA-B/GCp/GMPc soit impliquée dans le mécanisme de différenciation cardiaque puisque l’abolition du GMPc médiée par le GCp potentialise la différenciation cardiaque et il semblerait que cette voie de signalisation soit additive de la voie de signalisation induite par l’OT, NO/GCs/GMPc, puisque l’ajout de l’OT à l’antagoniste A71915 stimule plus fortement la différenciation cardiaque que l’OT ou l’A71915 seuls. Cela suggère que l’effet thérapeutique des peptides natriurétiques observé dans la défaillance cardiaque ainsi que les propriétés vasodilatatrices de certains antagonistes des récepteurs peptidiques natriurétiques inclus la stimulation de la différenciation des cellules souches en cardiomyocytes. Cela laisse donc à penser que les peptides natriurétiques ou les antagonistes des récepteurs peptidiques natriurétiques pourraient être une alternative très intéressante dans la thérapie cellulaire visant à induire la régénération cardiovasculaire.

Atrial natriuretic peptides: reproducibility of renal effects and response of liver blood flow.

To assess the variability of the response to exogenous atrial natriuretic peptide (ANP), it was infused at the rate of 1 microgram/min for 2 h in 6 salt-loaded normal volunteers under controlled conditions on 2 occasions at an interval of 1 week. The effect on solute excretion and the haemodynamic and endocrine actions were highly reproducible. The constant ANP infusion caused a delayed and prolonged excretion of sodium, chloride and calcium, no change in potassium or phosphate excretion or in glomerular filtration rate but a marked decrease in renal plasma flow. Blood pressure, heart rate and the plasma levels of angiotensin II, aldosterone, arginine vasopressin and plasma renin activity were unaltered. The effect of a 2-h infusion of ANP 0.5 microgram/min or its vehicle on apparent hepatic blood flow (HBF) was also studied in 14 normal volunteers by measuring the indocyanine green clearance. A 21% decrease in HBF was observed in subjects who received the ANP infusion (p less than 0.01 vs vehicle). Thus, ANP infused at a dose that did not lower blood pressure decreased both renal and liver blood flow in normotensive volunteers. The renal and endocrine responses to ANP were reproducible over a 1-week interval.