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Stellar physics
Results: 1072

#	Item
261	Data Analysis of the T Tauri Star V1331 Cyg Joshua Torres, Richard Olenick Ph.D, University of Dallas Submitted in partial fulfillment of the Bachelor of Science degree at Add to Reading List Source URL: phys.udallas.edu Language: English - Date: 2006-10-17 17:05:12 Stellar astronomy Light sources Star formation Star types Stellar evolution Protostar Star Interstellar medium Molecular cloud Astronomy Physics Astrophysics
262	Monday, June 02, 2003 A dense cluster of thousands of bright young stars in the nearby galaxy NGC 5253 is hidden in a "cloak of invisibility", which it appears to hold by its great gravitational attraction, says a team o Add to Reading List Source URL: www.astro.tau.ac.il Language: English - Date: 2003-06-08 02:23:32 Physical cosmology Astrophysics Star Cosmic distance ladder Modified Newtonian dynamics Comet Galaxy Physics Stellar astronomy Astronomy
263	MNRAS 446, 4205–doi:mnras/stu2398 A multiwavelength study of the M dwarf binary YY Geminorum C. J. Butler,1‹ N. Erkan,2 E. Budding,3 J. G. Doyle,1 B. Foing,4 G. E. Bromage,5 Add to Reading List Source URL: star.arm.ac.uk Language: English - Date: 2015-01-05 04:43:59 Light sources Plasma physics Sun Space plasmas Stellar astronomy Corona RS Canum Venaticorum variable Solar flare Cosmic distance ladder Astronomy Space Physics
264	Life of a Star An Interview with a White Dwarf, Sol Reflection Problems PAGE: Hang on, let’s talk about that balance. SOL: Before I could collapse, I had to satisfy a few conditions: Conservation of energy – the kine Add to Reading List Source URL: www.as.utexas.edu Language: English - Date: 2007-06-22 15:44:42 Stellar evolution Space Stellar astronomy Light sources Astrophysics Star Sun White dwarf Luminosity Astronomy Physics Star types
265	THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE? The stars are spheres of hot gas. Most of them shine because they are fusing hydrogen into helium in their central parts. In this problem we use concepts of both classica Add to Reading List Source URL: www.jyu.fi Language: English - Date: 2009-09-10 04:09:08 Nuclear chemistry Nuclear physics Chemical elements Stellar astronomy Astrophysics Nuclear fusion Helium Star Electron Physics Chemistry Matter
266	Studying White Dwarfs Event Lesson Plan version 1 Studying White Dwarfs at McDonald Observatory Event Lesson Plan for Argos Online Lock-in Add to Reading List Source URL: www.as.utexas.edu Language: English - Date: 2007-06-22 11:37:09 Matter Dark matter Star types Stellar evolution Plasma physics White dwarf Stellar classification Star Pulsating white dwarf Astronomy Space Stellar astronomy
267	Life of a Star An Interview with a White Dwarf, Sol Introduction This activity is an opportunity for students to apply their knowledge and understanding of the gas law, conservation of energy, and forces to stellar evolu Add to Reading List Source URL: outreach.as.utexas.edu Language: English - Date: 2007-02-01 11:53:17 Stellar evolution Star types Stellar astronomy Light sources Space plasmas Helium flash Star Sun Supernova Astronomy Physics Space
268	Star formation: basic physics Lecture 2 supplementary images Daniel Price – 26 – Add to Reading List Source URL: users.monash.edu.au Language: English - Date: 2010-03-02 21:47:52 Universe Star types Dark matter Initial mass function Open clusters Brown dwarf Star cluster Orion Nebula Star Astronomy Stellar astronomy Space
269	PHD QUALIFY EXAMINATION — STELLAR ASTROPHYSICS March, points) A low mass sequence star has mass M , radius R and eﬀective surface temperature Teﬀ . (a) (15 points) Find the average time a photon reside Add to Reading List Source URL: www.astro.ncu.edu.tw Language: English - Date: 2014-05-12 00:06:46 Stellar evolution Space Stellar astronomy Light sources Hertzsprung-Russell classifications Star White dwarf Nuclear fusion Main sequence Astronomy Physics Star types
270	Pair-Instability Black Hole Formation and You! Simon Porter September 21, 2007 Hyper-Large Pop III Stars Add to Reading List Source URL: www.asu.edu Language: English - Date: 2007-09-28 02:11:01 Matter Light sources Stellar astronomy Hypernovae Pair-instability supernova Neutrino Supernova Star Cosmic neutrino background Physics Astronomy Supernovae

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