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Stellar physics
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171	Joshua Edward Barnes – Curriculum Vitae Date & place of birth: August 30, 1956; London, England. Citizenship: United States of America. Address: Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA. Add to Reading List Source URL: www.ifa.hawaii.edu Language: English - Date: 2014-01-12 10:42:10 Galaxies Galaxy formation and evolution Stellar evolution Galaxy merger Interacting galaxy Starburst galaxy Elliptical galaxy Dark matter Bulge Astronomy Physics Extragalactic astronomy
172	Measurement of Spin-Orbit Alignment in an Extrasolar Planetary System Mark Richardson Outline Add to Reading List Source URL: www.asu.edu Language: English - Date: 2009-10-03 02:41:53 Celestial mechanics Rotation Conservation laws Angular momentum Formation and evolution of the Solar System Orbit Star Spin Stellar rotation Physics Rotational symmetry Stellar astronomy
173	A The Astrophysical Journal, 616:339–345, 2004 November 20 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. PHOTOMETRY OF SN 2002ic AND IMPLICATIONS FOR THE PROGENITOR MASS-LOSS HISTO Add to Reading List Source URL: hpwren.ucsd.edu Language: English - Date: 2006-03-14 17:26:55 Standard candles Physics Stellar evolution Supernova Type Ia supernova Cosmic distance ladder Type II supernova SN 2002cx SN 2008ha Supernovae Astronomy Astrophysics
174	Astronomy & Astrophysics A&A 559, L7DOI: Add to Reading List Source URL: www.aanda.org Language: English Standard candles Light sources Stellar evolution Star types Cosmic distance ladder Physical cosmology Supernova Star White dwarf Astronomy Astrophysics Physics
175	Astronomy & Astrophysics A&A 570, L9DOI: Add to Reading List Source URL: www.aanda.org Language: English Space X-ray astronomy Photoevaporation Young stellar object Corona Extreme ultraviolet Very Large Array TW Hydrae Stellar classification Physics Astronomy Plasma physics
176	Question 4. Starting from radiative transfer equation, suppose the source function is a linear a b ,v function of vertical optical depth S ,v (a) Please explain what is limb darkening effect using the surface intensiti Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Physical quantities Star Limb darkening Jeans instability Free-fall time Magnetic field Mass James Hopwood Jeans Physics Stellar astronomy Astrophysics
177	Stars continued Notes compiled by Paul Woodward Add to Reading List Source URL: www.lcse.umn.edu Language: English - Date: 2015-04-03 23:00:56 Nuclear fusion Light sources Stellar evolution Nuclear physics Astrophysics Degenerate matter Star Supernova Helium Physics Matter Chemistry
178	Astronomy & Astrophysics A&A 570, L4DOI: Add to Reading List Source URL: www.aanda.org Language: English Astronomical spectroscopy Raman scattering Corona Stellar classification Å Spectroscopy Redshift Physics Astrophysics Astronomy
179	Homework questions for Ch. 4 Vol. IV Q1: Let’s define r0 as the point along a magnetic field line of the Astrospheric Magnetic Field (AMF) at which the field line is open to space by the stellar wind (this is the point Add to Reading List Source URL: www.heliophysics.ucar.edu Language: English - Date: 2014-07-14 17:17:11 Light sources Space plasmas Plasma physics Stellar astronomy Planetary science Aurora Magnetic field Sun Star Physics Electromagnetism Astronomy
180	MITCHELL INSTITUTE ASTRONOMY SEMINAR SERIES Chris Sneden, Ph.D. University of Texas at Austin Monday, February 16, 2015 \| 11:30 AM \| MIST M102 Add to Reading List Source URL: mitchell.tamu.edu Language: English - Date: 2015-02-13 16:30:46 Light sources Space Stellar astronomy Space plasmas Population II stars Star Chemical element Metallicity Supernova Astronomy Astrophysics Physics

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