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Stellar physics
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#	Item
561	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
562	Tracy L. Beck Research Interests and Plans My research interests are focused primarily on understanding the formation and evolution of young stars, their circumstellar disks and their associated outflows of material. I h Add to Reading List Source URL: www.stsci.edu Language: English - Date: 2009-05-21 15:11:00 Space Nebulae Stellar astronomy Young stellar object Herbig–Haro object Light sources Active galactic nucleus Gemini Observatory Polar jet Astronomy Star formation Physics
563	Draft version October 8, 2014 Preprint typeset using LATEX style emulateapj v[removed]arXiv:1410.1544v1 [astro-ph.GA] 6 Oct[removed]DISCOVERY OF CARBON RADIO RECOMBINATION LINES IN M82 Add to Reading List Source URL: arxiv.org Language: English - Date: 2014-10-07 20:32:17 LOFAR University of Groningen Astronomy Redshift Spectral line Stellar classification Infrared Electromagnetic radiation Physics Spectroscopy
564	Microsoft Word - CP jets astro_charté_ok en.docx Add to Reading List Source URL: www2.cnrs.fr Language: English - Date: 2014-10-20 03:41:15 Stellar astronomy Magnetism Dark matter Polar jet LULI Plasma Stellar magnetic field Star White dwarf Physics Astrophysics Black holes
565	Lecture 12 Advanced Stages of Stellar Evolution – II Silicon Burning and NSE The solution of reaction networks. Add to Reading List Source URL: www.ucolick.org Language: English - Date: 2011-05-10 17:17:19 Physics Neon-burning process Silicon-burning process Supernova Silicon Abundances of the elements Astrophysics Chemistry Nucleosynthesis
566	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
567	Einstein Fellowship Symposium Day 1 Oct[removed]Phillips Auditorium Add to Reading List Source URL: cxc.harvard.edu Language: English - Date: 2014-10-27 14:08:57 Space plasmas Stellar evolution Plasma physics Supernovae Fluid dynamics Supernova Magnetohydrodynamics Gamma-ray burst Galaxy formation and evolution Physics Astrophysics Astronomy
568	Einstein Fellowship Symposium, Oct[removed]Day 1 Agenda Session 1, 9:[removed]:40 9:20 - 9:40 Reinout van Weeren Add to Reading List Source URL: cxc.harvard.edu Language: English - Date: 2014-10-27 16:57:03 Space plasmas Stellar evolution Plasma physics Supernovae Fluid dynamics Supernova Magnetohydrodynamics Gamma-ray burst Galaxy formation and evolution Physics Astrophysics Astronomy
569	The Origin of Our Universe Number Puzzle About 14 billion years ago, our entire universe came into existence in an event called the 1)____________. Because this state of matter, energy, light, space and time were so unim Add to Reading List Source URL: spacemath.gsfc.nasa.gov Language: English - Date: 2013-08-21 12:07:44 Physical cosmology Light sources Space plasmas Universe Stellar evolution Big Bang Helium Galaxy Star Physics Astrophysics Astronomy
570	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

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