Active star formation_in_n11
Discovery of xray_emission_from_young_suns_in_the_small_magellaniccloud
Cosmology 2002/2003 - March1 The Luminosity Function See Math in Tecra 8100 Thanks for Dr. Paolo Saracco for the example of the L.F. Estimate with V max.
Stellar Evolution Stars evolve (change over time) because of GRAVITY! A star passes through phases, grouped as –Pre-Main Seq (birth) –Main Seq (MS)(life)
By Guido Chincarini H o =50 km/s/Mpc L * =3.2 10 10 L = -1.25 Mv =-26.78 Mbol =-26.85