Cryopreservation of human semen and prepared sperm: effects on motility parameters and DNA integrity

Objective: To investigate effects of cryopreservation on sperm motility and DNA integrity. Design: Pre-cryopreservation and post-cryopreservation analysis of motility and DNA integrity of semen and prepared sperm samples. Setting: A hospital andrology laboratory. Patient(s): Forty men attending the Regional Fertility Centre, Belfast, Northern Ireland. Intervention(s): Each sample was divided, and an aliquot was frozen unprepared. Remaining aliquots were prepared by Percoll density centrifugation (95.0:47.5) or direct swim-up procedure and divided into aliquots to allow direct comparison of fresh and frozen semen and prepared sperm (frozen with or without the addition of seminal plasma) from the same ejaculate. Samples were frozen by static-phase vapor cooling and being plunged into liquid nitrogen. Thawing was carried out at room temperature. Main Outcome Measure(s): Sperm DNA integrity was determined using a modified alkaline single cell gel electrophoresis (comet) assay, and motility was determined using computer-assisted semen analysis. Result(s): Sperm frozen unprepared in seminal fluid appeared more resistant to freezing damage than frozen prepared sperm. Further improvements can be achieved by selecting out the subpopulation of sperm with best motility and DNA integrity and freezing these sperm in seminal plasma, making this the optimal procedure. Conclusion(s): Freezing sperm in seminal plasma improves postthaw motility and DNA integrity.

The VLT-FLAMES survey of massive stars: stellar parameters and rotational velocities in NGC 3293, NGC 4755 and NGC 6611

An analysis is presented of VLT-FLAMES spectroscopy for three Galactic clusters, NGC3293, NGC4755 and NGC6611. Non-LTE model atmosphere calculations have been used to estimate effective temperatures (from either the helium spectrum or the silicon ionization equilibrium) and gravities (from the hydrogen spectrum). Projected rotational velocities have been deduced from the helium spectrum (for fast and moderate rotators) or the metal line spectrum (for slow rotators). The origin of the low gravity estimates for apparently near main sequence objects is discussed and is related to the stellar rotational velocity. The atmospheric parameters have been used to estimate cluster distances (which are generally in good agreement with previous determinations) and these have been used to estimate stellar luminosities and evolutionary masses. The observed Hertzsprung-Russell diagrams are compared with theoretical predictions and some discrepancies including differences in the main sequence luminosities are discussed. Cluster ages have been deduced and evidence for non-coeval star formation is found for all three of the clusters. Projected rotational velocities for targets in the older clusters, NGC3293 and NGC4755, have been found to be systematically larger than those for the field, confirming recent results in other similar age clusters. The distribution of projected rotational velocities are consistent with a Gaussian distribution of intrinsic rotational velocities. For the relatively unevolved targets in the older clusters, NGC3293 and NGC4755, the peak of the velocity distribution would be 250 km s(-1) with a full-width-half-maximum of approximately 180 km s(-1). For NGC6611, the sample size is relatively small but implies a lower mean rotational velocity. This may be evidence for the spin-down effect due to angular momentum loss through stellar winds, although our results are consistent with those found for very young high mass stars. For all three clusters we deduce present day mass functions with Gamma-values in the range of -1.5 to -1.8, which are similar to other young stellar clusters in the Milky Way.

Analysis of parameters of haemostasis in pre-eclamptic, normotensive pregnant and non-pregnant women.

Pregnancy is characterized by a state of heightened coagulation, which is exacerbated in pathological conditions such as pre-eclampsia (PET). PET is further associated with abnormal maternal inflammation and increased circulating microparticles (MP); however, a mechanistic link between these pathological features has never been established. It is proposed in this thesis that abnormal maternal inflammation is causally linked to pro-coagulant trophoblast MP shedding via a mechanism mediated by the pro-inflammatory cytokine tumour necrosis factor alpha (TNF), thereby contributing to maternal coagulopathies associated with PET. Using thromboelastography (TEG) and standard laboratory tests, haemostatic function was evaluated in PET and normotensive subjects at delivery and post-partum. Furthermore, the effects of the menstrual cycle and oral contraceptive (OC) use on haemostatic function were assessed in non-pregnant subjects in order to understand their influence on post-partum haemostasis. Plasma TNF and pro-coagulant MP levels were evaluated in the pregnant subjects. Using chorionic villi explants from human term placentas, MPs were quantified after TNF administration. The pro-coagulant potential of placental MPs was evaluated by TEG by spiking whole-blood with medium containing MPs from chorionic villi. TEG identified increased whole-blood coagulability in PET subjects at delivery, demonstrating its increased sensitivity over standard laboratory tests at identifying haemostatic alterations associated with PET. Haemostatic alterations were normalized by six weeks post-partum. TEG also identified cyclic haemostatic variations associated with OC use. Chorionic villi treated with TNF (1 ng/ml) shed significantly more MPs than untreated placentas. MPs from chorionic villi increased the coagulability of whole-blood. Together, results provide evidence supporting the concept that abnormal maternal inflammation is causally linked to the development of maternal coagulopathies in pregnancy complications. Moreover, TEG may be superior to standard laboratory tests in evaluating haemostasis in pregnant and non-pregnant subjects.