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On the cobalt abundances of early-type stars
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 353, no 1, 335-338 p.Article in journal (Refereed) Published
Abstract [en]

Photographic region high-dispersion high signal-to-noise spectra of A and F main sequence band stars which exhibit modest rotation show Co I lines. In the hottest of these stars, we also found weak Co II lines whose abundances are consistent with those fr

Place, publisher, year, edition, pages
SPRINGER VERLAG , 2000. Vol. 353, no 1, 335-338 p.
Keyword [en]
stars : abundances; stars : chemically peculiar; DAO SPECTROGRAMS; A-STARS; EFFECTIVE TEMPERATURE; SURFACE GRAVITY; BETA PHOTOMETRY; B-STARS; DRACONIS; PECULIAR; HR-1094
Identifiers
URN: urn:nbn:se:uu:diva-36613OAI: oai:DiVA.org:uu-36613DiVA: diva2:64512
Note
Addresses: Adelman SJ, The Citadel, Dept Phys, 171 Moultrie St, Charleston, SC 29409 USA. The Citadel, Dept Phys, Charleston, SC 29409 USA. Natl Res Council Canada, Herzberg Inst Astrophys, Dominion Astrophys Observ, Victoria, BC V8X 4M6, Canada. BrandonAvailable from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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