1![PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS September, points) Consider a pure hydrogen stellar envelope at ρ = 10−8 g cm−1 and T = 20, 000 K. (a) (5 points) Calculate the relative populations of t PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS September, points) Consider a pure hydrogen stellar envelope at ρ = 10−8 g cm−1 and T = 20, 000 K. (a) (5 points) Calculate the relative populations of t](https://www.pdfsearch.io/img/4fd0a89b281ee262083d309764c05fbf.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
|
---|
2![Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 9:00–13:00, 31st May, points) Gravitational binding energy, dynamical timescale. Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 9:00–13:00, 31st May, points) Gravitational binding energy, dynamical timescale.](https://www.pdfsearch.io/img/0f8d502494ffcccd4c20c14432618dee.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
|
---|
3![Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 30th May, 2005 Please answer 5 out of the following 7 problemspoints) Institute of Astronomy, National Central University PHD QUALIFYING EXAMINATION — STELLAR ASTROPHYSICS 30th May, 2005 Please answer 5 out of the following 7 problemspoints)](https://www.pdfsearch.io/img/32e270e0aedd0cbe2ab0c80e6fbb2b48.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
|
---|
4![The physics of white dwarfs Increasingly sensitive and detailed astronomical observations coupled with calculations of the properties of matter under extreme conditions have given us new insights into their structure and The physics of white dwarfs Increasingly sensitive and detailed astronomical observations coupled with calculations of the properties of matter under extreme conditions have given us new insights into their structure and](https://www.pdfsearch.io/img/30f390dce5cfaef180f398f64168c3a9.jpg) | Add to Reading ListSource URL: astro.berkeley.eduLanguage: English - Date: 2012-11-04 13:12:40
|
---|
5![Overluminous supernovae push the Chandrasekhar limit Overluminous supernovae push the Chandrasekhar limit](https://www.pdfsearch.io/img/8ff885cb2625d946c8db8e6bfd7be652.jpg) | Add to Reading ListSource URL: astro.berkeley.eduLanguage: English - Date: 2012-11-04 13:10:18
|
---|
6![Standard Type Ia supernovae have a surprisingly large range of masses Standard Type Ia supernovae have a surprisingly large range of masses](https://www.pdfsearch.io/img/66ea01cc43c8b37c02758a250dc474ee.jpg) | Add to Reading ListSource URL: phys.orgLanguage: English - Date: 2015-03-03 22:24:53
|
---|
7![Chemical Evolution Chemical Evolution ](https://www.pdfsearch.io/img/5c861a8c2d12d51279a39f6bb2f79de5.jpg) | Add to Reading ListSource URL: www.cosmocomp.dur.ac.ukLanguage: English - Date: 2012-04-15 15:26:41
|
---|
8![Schonberg-Chandrasekhar Limit Isothermal cores, e.g., after core H burning
L(r) ~ 0 ~ dT/dr Schonberg-Chandrasekhar Limit Isothermal cores, e.g., after core H burning
L(r) ~ 0 ~ dT/dr](https://www.pdfsearch.io/img/e27f32f05518e45e427b47975afc52c6.jpg) | Add to Reading ListSource URL: www.astro.princeton.edu- Date: 2008-11-14 15:34:50
|
---|
9![Microsoft Word - white_dwarfs.doc Microsoft Word - white_dwarfs.doc](https://www.pdfsearch.io/img/0fd482ebc1048e2ad9126df2f699409a.jpg) | Add to Reading ListSource URL: www.chandra.harvard.eduLanguage: English - Date: 2008-01-29 13:13:39
|
---|
10![Microsoft Word - white_dwarfs.doc Microsoft Word - white_dwarfs.doc](https://www.pdfsearch.io/img/ab22f6e564bfdaf343f4bfaecafbc97f.jpg) | Add to Reading ListSource URL: chandra.si.eduLanguage: English - Date: 2008-01-29 13:13:39
|
---|