THE STELLAR INITIAL MASS FUNCTION: CONSTRAINTS FROM YOUNG CLUSTERS, AND THEORETICAL PERSPECTIVES MICHAEL R. MEYER University of Arizona, Steward Observatory FRED C. ADAMS

First Page		Document Content
Date: 2007-04-05 13:30:18 Stellar evolution Space Star types Star formation Initial mass function Star cluster Star Cosmic distance ladder White dwarf Astronomy Stellar astronomy Physics		THE STELLAR INITIAL MASS FUNCTION: CONSTRAINTS FROM YOUNG CLUSTERS, AND THEORETICAL PERSPECTIVES MICHAEL R. MEYER University of Arizona, Steward Observatory FRED C. ADAMS Add to Reading List Source URL: www.uapress.arizona.edu Download Document from Source Website File Size: 198,77 KB Share Document on Facebook

	Topical Lecture Week From Stars to Elements: Stellar Evolution DocID: 1uGPx - 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
	PDF Document DocID: 1rk6l - View Document
	A Mysterious Rash of Star Birth Image Credit: Gemini Observatory/AURA/T. Rector Gemini Observatory Legacy Image DocID: 1rcIl - View Document
	Astronomy & Astrophysics A&A 580, L3DOI: DocID: 1qQ0s - View Document