Your browser doesn't support javascript.
loading
Mostrar: 20 | 50 | 100
Resultados 1 - 3 de 3
Filtrar
Más filtros

Base de datos
Tipo de estudio
Tipo del documento
País de afiliación
Intervalo de año de publicación
2.
Theriogenology ; 77(6): 1186-97, 2012 Apr 01.
Artículo en Inglés | MEDLINE | ID: mdl-22153263

RESUMEN

This study investigated the effects of porcine granulocyte-macrophage colony-stimulating factor (pGM-CSF) on the developmental potential of porcine in vitro-fertilized (IVF) embryos in chemically and semidefined (with BSA) medium. In experiment 1, zygotes were treated with different concentrations of pGM-CSF (0, 2, 10, 100 ng/mL). The results indicated that 10 ng/mL pGM-CSF significantly (P < 0.05) increased blastocyst development and total cell number (15.1% and 53.5, respectively) compared with the control (6.1%, and 38.8, respectively). Comparing blastocyst formation, early and expanded blastocyst formation was significantly higher in the 10 ng/mL-pGM-CSF group than in the control on Days 6 and 7 of the culture period. However, there was no significant difference in cleavage rate. Experiment 2 demonstrated that pGM-CSF influenced the percentage of blastocyst formation and total cell number when pGM-CSF was added during Days 4 to 7 (14.6% and 53.9, respectively) or Days 0 to 7 (15.2% and 54.0, respectively) compared with the control (7.8% and 43.1, respectively) and compared with Days 0 to 3 (8.7% and 42.5, respectively). Similarly, early blastocyst formation rates were significantly higher at Days 4 to 7 than in the control, and expanded blastocyst formation was significantly higher at Days 4 to 7 or Days 0 to 7. No significant difference in cleavage rates appeared among the groups. In experiment 3, in the presence of BSA, pGM-CSF also increased the percentage of embryos that developed to the blastocyst stage and the total cell number (20.3% and 59.8, respectively) compared with the control (14.9% and 51.4, respectively), whereas there was no significant difference in cleavage rate. Experiment 4 found that the total cell number and the number of cells in the inner cell mass (ICM) were significantly increased compared with the control when zygotes were cultured in either porcine zygotic medium (PZM)-3 or PZM-4 supplemented with 10 ng/mL pGM-CSF. The number of trophectoderm (TE) cells was significantly higher in PZM-3 medium supplemented with pGM-CSF than in the control, and the number tended to increase (P = 0.058) in PZM-4 medium supplemented with pGM-CSF. The ratio of inner cell mass to trophectoderm cells was significantly higher in PZM-4 supplemented with 10 ng/mL pGM-CSF, but not in PZM-3. In experiment 5, it was found that the male pronuclear formation rate, monospermic penetration and sperm/oocyte were 95.4%, 37.2%, and 2.4, respectively. Together, these results suggest that pGM-CSF may have a physiological role in promoting the development of porcine preimplantation embryos and regulating cell viability and that addition of pGM-CSF to IVC medium at Days 4 to 7 or 0 to 7 improves the developmental potential of porcine IVF embryos.


Asunto(s)
Técnicas de Cultivo de Embriones/veterinaria , Embrión de Mamíferos/efectos de los fármacos , Desarrollo Embrionario/efectos de los fármacos , Fertilización In Vitro/veterinaria , Factor Estimulante de Colonias de Granulocitos y Macrófagos/farmacología , Porcinos/embriología , Animales , Femenino , Fertilización , Interacciones Espermatozoide-Óvulo
3.
Nature ; 476(7361): 421-4, 2011 Aug 24.
Artículo en Inglés | MEDLINE | ID: mdl-21866154

RESUMEN

Supermassive black holes have powerful gravitational fields with strong gradients that can destroy stars that get too close, producing a bright flare in ultraviolet and X-ray spectral regions from stellar debris that forms an accretion disk around the black hole. The aftermath of this process may have been seen several times over the past two decades in the form of sparsely sampled, slowly fading emission from distant galaxies, but the onset of the stellar disruption event has not hitherto been observed. Here we report observations of a bright X-ray flare from the extragalactic transient Swift J164449.3+573451. This source increased in brightness in the X-ray band by a factor of at least 10,000 since 1990 and by a factor of at least 100 since early 2010. We conclude that we have captured the onset of relativistic jet activity from a supermassive black hole. A companion paper comes to similar conclusions on the basis of radio observations. This event is probably due to the tidal disruption of a star falling into a supermassive black hole, but the detailed behaviour differs from current theoretical models of such events.

SELECCIÓN DE REFERENCIAS
DETALLE DE LA BÚSQUEDA