1![**TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** Radiation driven atmospheres of O-type stars: constraints on the mass–luminosity relation of **TITLE** ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS** Radiation driven atmospheres of O-type stars: constraints on the mass–luminosity relation of](https://www.pdfsearch.io/img/3d67c8838a6ba0d13c7c6e0a1d8179e7.jpg) | Add to Reading ListSource URL: www.usm.uni-muenchen.deLanguage: English - Date: 2002-02-06 06:35:03
|
---|
2![PHD QUALIFY EXAMINATION —GALACTIC AND EXTRAGALACTIC ASTROPHYSICS September, points) Calculate the order of magnitude of the Sunyaev-Zel’dovich effect for a typical cluster of galaxypoints) PHD QUALIFY EXAMINATION —GALACTIC AND EXTRAGALACTIC ASTROPHYSICS September, points) Calculate the order of magnitude of the Sunyaev-Zel’dovich effect for a typical cluster of galaxypoints)](https://www.pdfsearch.io/img/21606505f576e39244d20be61ac007e0.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
|
---|
3![Homework #1 1. The density of the interior of the sun is significantly larger than that of water. a) Provide a quantitative relation between the temperature and density of a star which indicates when we can treat it as a Homework #1 1. The density of the interior of the sun is significantly larger than that of water. a) Provide a quantitative relation between the temperature and density of a star which indicates when we can treat it as a](https://www.pdfsearch.io/img/03f2ee685f508eda69df981a24cfd899.jpg) | Add to Reading ListSource URL: astro.berkeley.eduLanguage: English - Date: 2013-01-28 21:05:13
|
---|
4![Shell Burning Red Giants Supergiants Asymptotic Giant Branch Paczynski Relation: (Core Mass-Luminosity) Shell Burning Red Giants Supergiants Asymptotic Giant Branch Paczynski Relation: (Core Mass-Luminosity)](https://www.pdfsearch.io/img/4193e3454893d5a8f3e354085a5d751a.jpg) | Add to Reading ListSource URL: www.astro.princeton.edu- Date: 2008-08-30 15:46:18
|
---|
5![The stochastic nature of stellar population modelling Miguel Cervi˜noa,b,c a Instituto arXiv:1312.0015v1 [astro-ph.IM] 29 Nov 2013 The stochastic nature of stellar population modelling Miguel Cervi˜noa,b,c a Instituto arXiv:1312.0015v1 [astro-ph.IM] 29 Nov 2013](https://www.pdfsearch.io/img/a0052e4bf91c00126e4dd234c543f6da.jpg) | Add to Reading ListSource URL: ned.ipac.caltech.eduLanguage: English - Date: 2014-06-27 19:04:16
|
---|