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CNO abundances in the quintuplet cluster M supergiant 5-7

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dc.contributor.author Ramirez, S. V. en_US
dc.contributor.author Sellgren, K. en_US
dc.contributor.author Blum, R. en_US
dc.contributor.author Terndrup, D. M. en_US
dc.date.accessioned 2004-09-22T18:12:08Z
dc.date.available 2004-09-22T18:12:08Z
dc.date.issued 2002-11-03 en_US
dc.identifier.citation Galactic Center Workshop 2002 en_US
dc.identifier.citation Kailua-Kona, HI, USA en_US
dc.identifier.clearanceno 03-1548 en_US
dc.identifier.uri http://hdl.handle.net/2014/11304
dc.description.abstract We present and analyze infrared spectra of the supergiant VR 5-7, in the Quintuplet cluster 30 pc from the Galactic center. Within the uncertainties, the [C/H],[N/H], and [O/H] abundances in this star are equal of Ori, a star which exhibits mixing of CNO processed elements, but distinct from the abundance patterns in IRS 7. en_US
dc.format.extent 2903081 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other stars Galactic Center en_US
dc.title CNO abundances in the quintuplet cluster M supergiant 5-7 en_US


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