Stellar astronomy - PDFSEARCH.IO - Document Search Engine

Stellar astronomy
Results: 2515

#	Item
551	Draft version March 31, 2015 Preprint typeset using LATEX style emulateapj vNATURE OF THE EXTREME ULTRALUMINOUS X-RAY SOURCES 3 Grzegorz Wiktorowicz1 , Malgorzata Sobolewska2 , Aleksander Sadowski Add to Reading List Source URL: arxiv.org Language: English - Date: 2015-03-30 20:33:59 Black holes Stellar astronomy Star types X-ray astronomy Astrophysics Ultraluminous X-ray source Eddington luminosity Accretion disc Intermediate-mass black hole Astronomy Space Physics
552	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: wise-obs.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
553	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
554	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
555	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
556	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
557	PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 122:347–353, 2010 March © 2010. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. The First Release of the CSTAR Point Source Cata Add to Reading List Source URL: mcba11.phys.unsw.edu.au Language: English - Date: 2010-03-07 23:39:30 Geography of Antarctica Space Stars Star catalogue Stellar astronomy Dome A Sloan Digital Sky Survey RAVE Magnitude Astronomy Observational astronomy Astronomical surveys
558	S C I E N C E ’ S C O M PA S S of the GalaxyYet it was not until the early 1980s that Oort’s picture, in which random stellar perturbations feed new long-period comets into the inner solar system, was overturn Add to Reading List Source URL: star.arm.ac.uk Language: English - Date: 2002-06-24 07:38:28 Comets Oort cloud Kuiper belt Asteroid Jupiter Minor planet Kreutz Sungrazers Damocloid asteroid Jupiter Barrier Solar System Astronomy Planetary science
559	Interview With a White Dwarf – Teacher Guide (Condensed Version) Introduction This activity is an opportunity for students to apply their knowledge and understanding of the gas law, conservation of energy, and forces t Add to Reading List Source URL: www.as.utexas.edu Language: English - Date: 2007-06-22 12:38:42 Star types Stellar evolution Stellar astronomy Planetary science Star Solar System White dwarf Planetary nebula Supernova Astronomy Space Light sources
560	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

UPDATE