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Astro-Physics
Results: 813

#	Item
111	SUMMARY IV: FUNDAMENTAL PRINCIPLES • Stars are self-gravitating bodies in dynamical equilibrium → balance of gravity and internal pressure forces (hydrostatic equilibrium); • stars lose energy by radiation from the Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-18 06:59:23
112	7. BINARY STARS (ZG: 12; CO: 7, 17) • most stars are members of binary systems or multiple systems (triples, quadruples, quintuplets, ...) 7.1 Classification • visual binaries: see the periodic wobbling of two stars Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-23 09:00:59
113	(2) low-mass stars: ideal-gas law, Kramer’s opacity law, i.e. ∝ T−3.5 Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-23 08:49:38
114	Hertzsprung-Russell (Colour-Magnitude) Diagram 2. Correlations between Stellar Properties 2.1 Mass-luminosity relationship (ZG: 12.2; CO: 7.3) • Most stars obey Ls = constant × Ms Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-18 06:48:49
115	Evolution of Massive Stars 6.3 EVOLUTION OF MASSIVE STARS (M > ∼ 13 M¯) (CO: 13.3) • massive stars continue to burn nuclear fuel beyond Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-12-01 08:01:38
116	Measuring cosmology with Supernovae Saul Perlmutter1 and Brian P. Schmidt2 1 arXiv:astro-phv1 18 Mar 2003 Add to Reading List Source URL: web.physics.ucsb.edu Language: English - Date: 2004-07-27 16:28:12
117	Daniel Lecoanet 6511 Telegraph Ave. #11, Oakland, CA-3950 http://astro.berkeley.edu/~lecoanet Add to Reading List Source URL: w.astro.berkeley.edu Language: English - Date: 2015-10-04 23:37:39 Fluid dynamics Physics Nature Continuum mechanics RayleighTaylor instability Geophysical fluid dynamics Gravity wave Convection Instability Wind wave Thermal conduction
118	CONVERSATIONS WITH SCIENTISTS Gianfranco Vidali: High-Risk Physics Much of the research that my colleagues and I do is highrisk research; it means we Add to Reading List Source URL: astro.syr.edu Language: English - Date: 2015-07-10 15:31:07
119	STELLAR STRUCTURE AND EVOLUTION 1. OBSERVABLE PROPERTIES OF STARS Basic large-scale observable properties: 1.1 LUMINOSITY (ZG: 11; CO: 3.1) (‘power’, [J/s=W]) Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-08 05:30:04
120	STRUCTURE OF THE SUN HELIOSEISMOLOGY (I) • The Sun is the only star for which we can measure internal properties → test of stellar structure theory Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2003-10-31 06:50:58

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