Chandrasekhar limit

Results: 18



#Item
1PHD 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

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
2Institute 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.

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
3Institute 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)

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46
4The 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

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Source URL: astro.berkeley.edu

Language: English - Date: 2012-11-04 13:12:40
5Overluminous supernovae push the Chandrasekhar limit

Overluminous supernovae push the Chandrasekhar limit

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Source URL: astro.berkeley.edu

Language: English - Date: 2012-11-04 13:10:18
6Standard Type Ia supernovae have a surprisingly large range of masses

Standard Type Ia supernovae have a surprisingly large range of masses

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Source URL: phys.org

Language: English - Date: 2015-03-03 22:24:53
7Chemical Evolution    

Chemical Evolution    

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Source URL: www.cosmocomp.dur.ac.uk

Language: English - Date: 2012-04-15 15:26:41
8Schonberg-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

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Source URL: www.astro.princeton.edu

- Date: 2008-11-14 15:34:50
    9Microsoft Word - white_dwarfs.doc

    Microsoft Word - white_dwarfs.doc

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    Source URL: www.chandra.harvard.edu

    Language: English - Date: 2008-01-29 13:13:39
    10Microsoft Word - white_dwarfs.doc

    Microsoft Word - white_dwarfs.doc

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    Source URL: chandra.si.edu

    Language: English - Date: 2008-01-29 13:13:39