×
+ All Categories
Log in
English
Français
Español
Deutsch
The top documents tagged [chandrasekhar mass limit]
Home >
chandrasekhar mass limit
Lecture 20 White dwarfs. Sirius B Wobble in the position of Sirius A led to the prediction of an unseen companion. Sirius BSirius A M/M Sun 1.0532.3 L/L.
215 views
1 Endpoints of stellar evolution The end of stellar evolution is an inert core of spent fuel that cannot maintain gas pressure to balance gravity Chandrasekhar.
215 views
Stellar Physics 2 Multiple Choice Questions. Test Question Does this quiz work? A.Yes B.No.
231 views
Lecture 21
31 views
X-ray Studies of Supernova Remnants Una Hwang (NASA/GSFC, JHU) X-ray Astronomy School 2007 George Washington University.
220 views
Credit: O. Krause (Steward Obs.) et al., SSC, JPL, Caltech, NASA South Africa and the SDSS-II Supernova Survey Ed Elson (SAAO/NASSP) Bruce Bassett (SAAO/ICG)
215 views