BB 1,2 H 3,4 He 7 Li Intergalactic medium Interstellar medium Galaxy formation inflowGal. winds, stripping, mergers Cosmic rays Small stars D, Li Middling.
Young stars in the nearest solar neighbourhood Oct 24, 2001 The Gould Belt and other large star forming complexes 1 Young stars in the nearest solar neighbourhood.
"Planet Formation in Dense Star Clusters" presented by Dr. Henry Throop (University of Pretoria)
Tracing evolution of_dust_in_eagle_nebula
Superwind phenomenon in_m82
Fluorescence and resonant ionization in astrophysical plasmas, with emphasis on and examples from the star Eta Carinae
Hydrogen Burning and Pulsations on Low Mass Helium Core White Dwarfs Justin D. R. Steinfadt Lars Bildsten UCSB Wild Stars in the Wild West II 14th North.
Stellar Evolution. Evolution on the Main Sequence Zero-Age Main Sequence (ZAMS) MS evolution Development of an isothermal core: dT/dr = (3/4ac) ( r/T.
Massive Stars live shorter lives. Low mass stars live longest. 1.Gravity contracts the Hydrogen gas 2. Gas Spins 3. Gas Heats 4. Protostar Stage 5. Fusion.
The Group of Bootis Stars Dr. Ernst Paunzen Institute for Astronomy University of Vienna.
Module : Activity 2: From After the ZAMS Module 8: Life on the Main Sequence Swinburne Online Education Exploring Stars and the Milky Way © Swinburne University.
M. Shara Sept. 26, 2007 Planets, White Dwarfs, Cataclysmic Variables and SNIa in Star Clusters: Changing the Rules Mike Shara American Museum of Natural.