Sobrevida y factores relacionados con reintervención en pacientes tratados con valvuloplastia aórtica con balón en la Fundación Cardioinfantil

Introducción: La valvuloplastía aórtica con balón (VAB) es el procedimiento de elección para el manejo de La estenosis valvular aórtica en pediatría. La mortalidad y la supervivencia libre de reintervenciones no han sido evaluadas en Colombia. Objetivo: Determinar la sobrevida global y los factores asociados de reintervención valvular aórtica (RVA) en los pacientes tratados con VAB en la Fundación Cardio infantil – Instituto de Cardiología entre febrero del 2005 y marzo del 2013. Métodos: estudio estudio analítico de cohorte Resultados: Se evaluaron 69 VAB. La edad promedio de realización fue de 74,89 meses. La relación hombre: mujer de 4:1. Un 30,5% de los pacientes tenían malformaciones cardiacas asociadas. Se presentaron complicaciones en 13% de las VAB. La presión sistólica del ventrículo izquierdo presento una reducción promedio de un 63,6%. Se siguieron el 81,2% de las VAB, encontrando a los 9 años de seguimiento, supervivencia de 89,2% y necesidad de RVA en 14,2% de las VAB, siendo más frecuentes en VAB con gradiente post-VAB mayor de 35 mmhg (p= 0.005), con un RR de 6.6. Los otros factores no mostraron relaciones estadísticamente significativas (edad, morfología valvular, malformaciones asociadas, insuficiencia aórtica post-VAB). Conclusiones: La VAB es eficaz en el manejo de la EVA congénita, con una mortalidad y supervivencia libre de RVA similares a las encontradas en estudios previamente publicados. El gradiente post VAB mayor de 35 mm hg fue el único factor de riesgo que se correlacionó con la supervivencia libre de RVA.

Medidas de longitudes de ondas con red de difracción : práctica para sexto curso.

Se trata de medir longitudes de onda del espectro visible. El valor exacto es de 656 milimicras. Se puede comprobar que esta raya corresponde al salto electrónico entre la tercera y la segunda órbita, según la fórmula de Balmer y siendo la constante de Rydberg.

Discovery in IC10 of the farthest known symbiotic star

We report the discovery of the first known symbiotic star in IC10, a starburst galaxy belonging to the Local Group, at a distance of similar to 750 kpc. The symbiotic star was identified during a survey of emission-line objects. It shines at V = 24.62 +/- 0.04, V - R(C) = 2.77 +/- 0.05 and R(C) - I(C) = 2.39 +/- 0.02, and suffers from E(B-V) = 0.85 +/- 0.05 reddening. The spectrum of the cool component well matches that of solar neighbourhood M8III giants. The observed emission lines belong to Balmer series, [S II], [N II] and [O III]. They suggest a low electronic density, negligible optical depth effects and 35 000 < T(eff) < 90 000 K for the ionizing source. The spectrum of the new symbiotic star in IC10 is an almost perfect copy of that of Hen 2-147, a well-known Galactic symbiotic star and Mira.

The RAINY3D Code: The Treatment of Condensation in Nova Remnants during Nebular Phase

Classical nova remnants are important scenarios for improving the photoionization modeling. This work describes the pseudo-three-dimensional code RAINY3D, which drives the photoionization code Cloudy as a subroutine. Photoionization simulations of old nova remnants are also presented and discussed. In these simulations we analyze the effect of condensation in the remnant spectra. The condensed mass fraction affects the Balmer lines by a factor of greater than 4 when compared with homogeneous models, and this directly impacts the shell mass determination. The He II 4686/H beta ratio decreases by a factor of 10 in clumpy shells. These lines are also affected by the clump size and density distributions. The behavior of the strongest nebular line observed in nova remnants is also analyzed for heterogeneous shells. The gas diagnoses in novae ejecta are thought to be more accurate during the nebular phase, but we have determined that at this phase the matter distribution can strongly affect the derived shell physical properties and chemical abundances.

A cyclic bipolar wind in the interacting binary V 393 Scorpii

V393 Scorpii is a double periodic variable characterized by a relatively stable non-orbital photometric cycle of 253 d. Mennickent et al. argue for the presence of a massive optically thick disc around the more massive B-type component and describe the evolutionary stage of the system. In this paper, we analyse the behaviour of the main spectroscopic optical lines during the long non-orbital photometric cycle. We study the radial velocity of the donor determining its orbital elements and find a small but significant orbital eccentricity (e = 0.04). The donor spectral features are modelled and removed from the spectrum at every observing epoch using the light-curve model given by Mennickent et al. We find that the line emission is larger during eclipses and mostly comes from a bipolar wind. We also find that the long cycle is explained in terms of a modulation of the wind strength; the wind has a larger line and continuum emissivity at the high state. We report the discovery of highly variable chromospheric emission in the donor, as revealed by the Doppler maps of the emission lines Mg II 4481 and C I 6588. We discuss notable and some novel spectroscopic features like discrete absorption components, especially visible at blue depressed O I 7773 absorption wings during the second half-cycle, Balmer double emission with V/R curves showing 'Z-type' and 'S-type' excursions around secondary and main eclipses, respectively, and H beta emission wings extending up to +/- 2000 km s(-1). We also discuss possible causes for these phenomena and for their modulations with the long cycle.

Reversible microbial colonization of germ-free mice reveals the dynamics of IgA immune responses

The lower intestine of adult mammals is densely colonized with nonpathogenic (commensal) microbes. Gut bacteria induce protective immune responses, which ensure host-microbial mutualism. The continuous presence of commensal intestinal bacteria has made it difficult to study mucosal immune dynamics. Here, we report a reversible germ-free colonization system in mice that is independent of diet or antibiotic manipulation. A slow (more than 14 days) onset of a long-lived (half-life over 16 weeks), highly specific anticommensal immunoglobulin A (IgA) response in germ-free mice was observed. Ongoing commensal exposure in colonized mice rapidly abrogated this response. Sequential doses lacked a classical prime-boost effect seen in systemic vaccination, but specific IgA induction occurred as a stepwise response to current bacterial exposure, such that the antibody repertoire matched the existing commensal content.

Preliminary Experience in Treatment of Papillary and Macular Retinoblastoma: Evaluation of Local Control and Local Complications After Treatment with Linear Accelerator-Based Stereotactic Radiotherapy with Micromultileaf Collimator as Second-Line or Salvage Treatment after chemotherapy

To determine the local control and complication rates for children with papillary and/or macular retinoblastoma progressing after chemotherapy and undergoing stereotactic radiotherapy (SRT) with a micromultileaf collimator.

(106)Ruthenium brachytherapy for ciliary recurrence with supraciliary effusion in retinoblastoma

A 2-year-old boy with syndromic bilateral retinoblastoma resulting from a (del(13)(q12.3q14.3)) developed a recurrent tumor measuring 2.3 X 2.3 mm at the ora serrata 15 months following last treatment.

Modern cataract surgery for radiation-induced cataracts in retinoblastoma

Surgery of radiation-induced cataracts in children with retinoblastoma (RB) is a challenge as early intervention is weighted against the need to delay surgery until complete tumour control is obtained. This study analyses the safety and functional results of such surgery.