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Date: 2012-06-24 20:56:13 Space Stellar evolution Astrophysics Dark matter Star Anglo-Australian Telescope Stellar classification Metallicity Helium star Astronomy Star types Stellar astronomy		Microsoft Word - MANIFEST_newsletter_0110.doc Add to Reading List Source URL: 203.15.109.22 Download Document from Source Website File Size: 2,46 MB Share Document on Facebook

	T H E QUASAR 0805 + 046 AS A HELIUM-RICH S H E L L STAR Y . P. V A R S H N I Department of Physics, University of Ottawa, Canada K I N 6N5 (Received 3 July, 1985) Abstract. Within the framework of the plasma-laser star m DocID: 1uSVr - View Document
	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 DocID: 1pzX1 - View Document
	Physical parameters of helium-rich subdwarf B stars from spectral energy distributions? A. Ahmad and C. S. Jeffery Armagh Observatory, College Hill, Armagh BT61 9DG. N. Ireland. UK Received 15 JulyAccepted 02 Oct DocID: 1o3Dt - View Document
	Astronomy & Astrophysics manuscript no. Hg223 (DOI: will be inserted by hand later) October 3, 2005 Extreme helium stars: non-LTE matters DocID: 1nVOq - View Document
	c ESO 2005 Discovery of pulsation in a helium-rich subdwarf B star A. Ahmad and C. S. Jeﬀery Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland, UK DocID: 1n2ht - View Document