A comprehensive analysis of the cool RCB star DY Persei

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/33820

Title:	A comprehensive analysis of the cool RCB star DY Persei
Authors:	Zacs,L.;Mondal,S.;Chen,W. P.;Pugach,A. F.;Musaev,F. A.;Alksnis,O.
Contributors:	天文研究所
Keywords:	CORONAE-BOREALIS STARS;CARBON STARS;SPECTROSCOPY;KINEMATICS;DISK
Date:	2007
Issue Date:	2010-07-07 11:49:46 (UTC+8)
Publisher:	中央大學
Abstract:	Context. Theoretically, the number of cool Galactic R Coronae Borealis stars (RCBs) should be greater than the warm RCBs, however to date, only a few candidates have been detected. Aims. Observations of the extremely cool RCB candidate, DY Per, and the an
Relation:	ASTRONOMY & ASTROPHYSICS
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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