Lithium abundances in the α Per cluster

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DC Field	Value	Language
dc.contributor.author	Mallik, S. G. V	-
dc.contributor.author	Balachandran, S. C	-
dc.contributor.author	Lambert, D. L	-
dc.date.accessioned	2010-11-25T16:18:38Z	-
dc.date.available	2010-11-25T16:18:38Z	-
dc.date.issued	2010-04	-
dc.identifier.citation	C. Charbonnel, M. Tosi, F. Primas & C. Chiappini, eds., Light Elements in the Universe, Proceedings IAU Symposium No. 268, 2009, pp. 339-340	en
dc.identifier.uri	http://hdl.handle.net/2248/5266	-
dc.description	Restricted Access	en
dc.description.abstract	As a sequel to the Li observations by Balachandran, Lambert & Stauffer (1988, 1996) in 35 stars of the 50 Myr old cluster α Persei, we have obtained and analyzed high resolution spectra of another 51 stars. Following a reconsideration of the cluster membership of the stars (Prosser 1992, Makarov 2006, Mermilliod et al. 2008, and Patience et al. 2002), we discuss the Li abundances for 70 stars. With our larger sample, we reexamine the question of whether the scatter in Li abundance at a given Teff seen in young clusters at cool temperatures is real or not.	en
dc.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.ispartofseries	IAU Symposium and Colloquium Proceedings Series; Vol. 268	-
dc.relation.uri	http://dx.doi.org/10.1017/S1743921310004370	en
dc.rights	© Cambridge University Press	en
dc.subject	Galaxy: open clusters	en
dc.subject	Stars: abundances	en
dc.title	Lithium abundances in the α Per cluster	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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