Ever since the first fading counterpart of Gamma Ray Burst (GRB) was discovered in 1997 there had been tremendous progress in our understanding of GRBs both in observation and theory.
The understanding of the nature of AGNs and the galaxies hosting them belongs to one of the most interesting topics of modern astrophysical research.
Wednesday, July 3, 2002 - 14:00
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The inner part of the rotation curve is crucial in determining the nature of the dark matter. The shape of the dark spherical halo is determined by the central density and the core radius.
Tuesday, June 25, 2002 - 14:00
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Tbd
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Wednesday, June 19, 2002 - 19:00
Conferenciante:
Dr. Fernando Moreno
Filiación:
IAA-CSIC
Wednesday, June 12, 2002 - 14:00
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The dynamics of stellars systems is fully specified by its distribution function - the phase density of its consistuent stars - and the form of the gravitational potential that binds it together.
Monday, May 27, 2002 - 14:00
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Se han modelado quimicamente 4 galaxias enanas esferoidales (dSph) satelites locales a partir de historias de formacion estelar obtenidas de sus diagramas HR.
Friday, May 24, 2002 - 14:00
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Because of their low gravitational energies dwarf galaxies are greatly exposed to energetical influences from internal and external sources.
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Thursday, May 23, 2002 - 19:00
Conferenciante:
Dr. Francisco Anguita
Filiación:
UCM
Friday, May 17, 2002 - 14:00
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The availability of Hipparcos data has revolutionized astrometry. The impact has been felt more strongly in those fields where there is a significant number of objects within 200 pc, which corresponds to the maximum distance at which individual Hipparcos parallaxes can be considered accurate.
Tuesday, May 14, 2002 - 14:00
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We present a simple phenomenological model of feedback in early-type galaxies that tracks the evolution of the gas content, metallicity and temperature.
Friday, May 10, 2002 - 14:00
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Tidal Dwarf Galaxies (TDGs) are created during a violent interaction of galaxies containing at least one spiral. Atomic hydrogen is torn off a spiral and star formation takes place in this gas which accumulates at the ends of tidal tails.
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Thursday, April 25, 2002 - 19:00
Conferenciante:
Dr. Emilio Alfaro
Filiación:
IAA-CSIC
Thursday, April 25, 2002 - 14:00
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I will summarize the results of our recently completed HST/WFPC2 I-band survey of a sample of 77 nearby, late-type spiral galaxies with low inclination. The main purpose of this catalog is to study the frequency and properties of nuclear star clusters in this class of galaxies.
Wednesday, April 24, 2002 - 14:00
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Tbd
Wednesday, April 17, 2002 - 14:00
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Tbd
Tuesday, April 16, 2002 - 14:00
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El proyecto ALMA exigirá grandes esfuerzos tanto en el dominio técnico como en el de la modelización que deberá simular o tratar ciertos efectos.
Tuesday, April 2, 2002 - 14:00
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In hierarchical clustering scenarios of galaxy formation, such as cold dark matter-dominated cosmologies (White and Rees 1978), dwarf galaxies should have formed prior to the epoch of giant galaxy formation and would be the building blocks of larger galaxies.
Wednesday, March 20, 2002 - 13:00
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Tbd
Wednesday, March 13, 2002 - 13:00
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En esta charla voy a revisar la evolución del 4He en el Universo, con un énfasis particular en la determinación de la abundancia de Helio primordial Y_P y sus implicaciones cosmológicas. Discutiré las determinaciones más recientes de Y_P, y las incertidumbres que las afectan.