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Luminosities and temperatures of the reddest stars in three LMC clusters

Frogel, Jay A. and Persson, S. E. and Cohen, Judith G. (1980) Luminosities and temperatures of the reddest stars in three LMC clusters. Astrophysical Journal, 239 . pp. 495-501. ISSN 0004-637X. doi:10.1086/158133. https://resolver.caltech.edu/CaltechAUTHORS:20190531-091630459

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Abstract

Infrared observations in the 1.2-2.2 µm region are presented for 12 of the reddest stars in the Large Magellanic Cloud (LMC) clusters NGC 1783,1846, and 1978. Seven of the stars, which are carbon stars, are photometrically indistinguishable from carbon stars in the general field of the LMC. Bolometric magnitudes and temperatures are derived from the infrared data. The average bolometric magnitude of the carbon stars is —4.9, which is about two magnitudes fainter than previously published values, but still high enough to require that these stars are asymptotic giant branch stars. The most luminous M-type stars in these clusters are warmer and perhaps more luminous than the giant branches of metal-rich Galactic globular clusters, in agreement with Hodge’s results based on UBV photometry. The location of the M-type stars may present some problems for recent giant branch model calculations.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/158133DOIArticle
http://adsabs.harvard.edu/abs/1980ApJ...239..495FADSArticle
ORCID:
AuthorORCID
Cohen, Judith G.0000-0002-8039-4673
Additional Information:© American Astronomical Society • Provided by the NASA Astrophysics Data System. Received 1979 August 28; accepted 1980 January 22. Cerro Tololo Inter-American Observatory is supported by the National Science Foundation under contract No. AST 78-27879. J. A. F. would like to thank J. Baldwin and J. Elias for assistance with the 4 m observations and several of his colleagues at CTIO for useful comments on a draft of this paper. We are grateful to J. Mould and A. Aaronson for discussing their data with us before publication and for some valuable criticism of the present paper. We appreciate the continuing interest of V. M. Blanco in this project and the use, before publication, of his finding charts and coordinates.
Funders:
Funding AgencyGrant Number
NSFAST 78-27879
Subject Keywords:clusters : open — galaxies : Magellanic Clouds — stars : late-type — stars: luminosities
DOI:10.1086/158133
Record Number:CaltechAUTHORS:20190531-091630459
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190531-091630459
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95967
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:31 May 2019 20:47
Last Modified:16 Nov 2021 17:17

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