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The top documents tagged [stellar winds]

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
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
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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
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
215 views
"Planet Formation in Dense Star Clusters" presented by Dr. Henry Throop (University of Pretoria)
"Planet Formation in Dense Star Clusters" presented by Dr. Henry Throop (University of Pretoria)
350 views
Tracing evolution of_dust_in_eagle_nebula
Tracing evolution of_dust_in_eagle_nebula
9.738 views
Superwind phenomenon in_m82
Superwind phenomenon in_m82
4.361 views
Fluorescence and resonant ionization in astrophysical plasmas, with emphasis on and examples from the star Eta Carinae
Fluorescence and resonant ionization in astrophysical plasmas, with emphasis on and examples from the star Eta Carinae
428 views
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
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
215 views
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
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
230 views
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
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
213 views
The Group of Bootis Stars Dr. Ernst Paunzen Institute for Astronomy University of Vienna
The Group of Bootis Stars Dr. Ernst Paunzen Institute for Astronomy University of Vienna
222 views
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
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
219 views
M. Shara Sept. 26, 2007 Planets, White Dwarfs, Cataclysmic Variables and SNIa in Star Clusters: Changing the Rules Mike Shara American Museum of Natural
M. Shara Sept. 26, 2007 Planets, White Dwarfs, Cataclysmic Variables and SNIa in Star Clusters: Changing the Rules Mike Shara American Museum of Natural
216 views