Curriculum Vitae 1 Curriculum Vitae Patrick Young

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Date: 2014-08-25 19:22:51 Astrophysics Stellar evolution Light sources Nuclear physics Supernova Nucleosynthesis Main sequence Astronomy Star Nuclear astrophysics		Curriculum Vitae 1 Curriculum Vitae Patrick Young Add to Reading List Source URL: bahamut.sese.asu.edu Download Document from Source Website File Size: 105,65 KB Share Document on Facebook

	The Astrophysical Journal, 579:800–809, 2002 November 10 # 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A. LIMITS ON CHROMOSPHERES AND CONVECTION AMONG THE MAIN-SEQUENCE A STARS1 Theodor DocID: 1vnUK - View Document
	Astronomy Assessment and TPS Questions: Star Formation and Lifetimes The total main sequence lifetime of stars like the Sun is about 1 million years. DocID: 1uAWB - View Document
	SCHEDULE OF PRESENTATIONS 9:00-10:15 Session I— Pre-main sequence objects and binaries The Infrared Excess in the Eclipse of KH 15D Scott Allen, Vassar ‘12 Short Timescale Variations in the Spectrum of Beta Lyrae Lau DocID: 1umOK - View Document
	Astronomy Assessment and TPS Questions: Stellar Evolution In a main sequence star, gravitational collapse is balanced by convection of stellar material from the core. DocID: 1tMJF - View Document
	Astronomy Assessment and TPS Questions: Binary Stars From which binary star system (made up of two main sequence stars) described below would an Earth observer detect the least amount of total light? When a star with an DocID: 1tEv2 - View Document