Stellar structure - PDFSEARCH.IO - Document Search Engine

Stellar structure
Results: 127

#	Item
71	A The Astrophysical Journal, 637:811–822, 2006 February 1 # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE CIRCUMSTELLAR STRUCTURE OF THE CLASS I PROTOSTAR TMC-1 (IRAS 04381+2540) Add to Reading List Source URL: terryhancock.narya.net Language: English - Date: 2012-03-09 18:23:00 Space Star types T Tauri stars Nebulae T Tauri Star Protostar Free-fall time Circumstellar disk Stellar astronomy Astronomy Star formation
72	Mon. Not. R. Astron. Soc. 000, 1–[removed]Printed 13 April[removed]MN LaTEX style file v2.2) Add to Reading List Source URL: www.zora.uzh.ch Language: English - Date: 2011-03-15 07:11:12 Galaxies Large-scale structure of the cosmos Stellar evolution Physical cosmology Space plasmas Active galactic nucleus Galaxy groups and clusters Quasar Dark matter Astronomy Physics Space
73	Black Hole Masses in the Largest and Smallest Systems Karl Gebhardt (UTexas) The original papers on the BH correlations suggest that the intrinsic Add to Reading List Source URL: www.noao.edu Language: English - Date: 2009-06-30 16:54:39 Astroparticle physics Stellar astronomy Dark matter Large-scale structure of the cosmos Globular cluster M87 Star Physics Astronomy Galaxies
74	1975ApJ...199L..19T THE ASTROPHYSICAL JOURNAL, 199: Li 9-L24, 197 5 J u]y 1 © 1975. The American Astronomical Society. All rights reserved. Printed in U.S.A. Add to Reading List Source URL: authors.library.caltech.edu Language: English - Date: 2014-07-01 10:27:42 Space Universe Stellar evolution Light sources Exotic matter Star Stellar structure White dwarf Supergiant Star types Astronomy Stellar astronomy
75	General Description Guidelines Galaxies Did you use direct or averted vision? What is the overall shape? Is the core noticeable, compact, stellar ? Can structure be seen in the galaxy, mottling, Add to Reading List Source URL: www.astronomylogs.com Language: English - Date: 2009-07-19 17:08:06 Globular cluster Space Orion arm Messier objects Universe Astronomy Nebula Star
76	Mon. Not. R. Astron. Soc. 000, 000–[removed]Printed 13 April[removed]MN LATEX style file v2.2) Add to Reading List Source URL: www.zora.uzh.ch Language: English - Date: 2012-01-09 10:34:20 Physical cosmology Stellar evolution Local Group Galaxies Spiral galaxies Galaxy formation and evolution Dark matter Structure formation Milky Way Astronomy Physics Space
77	Poster Abstracts CosmoComp/Charm 2013 spring school Radiative transfer treatments for astrophysical applications Andreas bauer - Studying reionization using GPUs We have implemented a photon conserving radiative transfer Add to Reading List Source URL: cosmocompcharmschool2013.strw.leidenuniv.nl Language: English - Date: 2013-05-23 06:52:22 Physical cosmology Stellar astronomy Light sources Galaxy Spiral galaxy Structure formation Interstellar medium Redshift Active galactic nucleus Astronomy Physics Space
78	Homework # 31 1. Small amounts of Deuterium are made in the Big Bang. D is destroyed in the interiors of stars via the reaction p + D → 3 He + γ. The S value for D-burning is 2.5 × 10−4 keVbarn, each reaction relea Add to Reading List Source URL: astro.berkeley.edu Language: English - Date: 2013-03-06 13:06:52 Chemistry Stellar astronomy Star types Nuclear fusion Light sources Stellar structure CNO cycle Star Stellar classification Physics Astronomy Stellar evolution
79	Homework #2 1. There are two ways to estimate the energy carried by convection. The first is that the energy flux is Fc ≈ 1/2ρvc3 ≡ Fc,1 where vc is the characteristic velocity of the convective motions. This is the Add to Reading List Source URL: astro.berkeley.edu Language: English - Date: 2013-02-12 20:41:00 Physics Light sources Atmospheric thermodynamics Stellar structure Astrophysics Convection zone Convective overshoot Atmospheric convection Convection Meteorology Atmospheric sciences Stellar astronomy
80	5 Cold accretion flows and the nature of high column density H i absorption at redshift 3 Simulations predict that galaxies grow primarily through the accretion of gas that has not gone through an accretion shock near th Add to Reading List Source URL: home.strw.leidenuniv.nl Language: English - Date: 2012-03-13 09:15:30 Large-scale structure of the cosmos Physical cosmology Stellar evolution Astronomical objects Galaxy Dark matter Interstellar medium Star formation Quasar Physics Astronomy Astrophysics

UPDATE