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The clusters of M33

Cohen, J. G. and Persson, S. E. and Searle, L. (1984) The clusters of M33. Astrophysical Journal, 281 . pp. 141-147. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190531-091632901

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Abstract

A selection of clusters in M33 is studied using three different observational techniques which give consistent quantitative results. M33 contains clusters which resemble galactic globular clusters as well as clusters as young as 10^8 years; the luminous clusters thus have an age range similar to those of the Magellanic Clouds rather than those of our Galaxy or M31. The four true globular clusters in our sample are all more metal poor than 47 Tuc. Based on limited data, the carbon star contribution to the integrated infrared light of the intermediate age clusters in M33 is approximately the same as in the intermediate age clusters in the Magellanic Clouds.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/162083DOIArticle
http://adsabs.harvard.edu/abs/1984ApJ...281..141CADSArticle
ORCID:
AuthorORCID
Cohen, J. G.0000-0002-8039-4673
Additional Information:© American Astronomical Society • Provided by the NASA Astrophysics Data System. Received 1983 June 17; accepted 1983 December 1.
Subject Keywords:clusters: globular — clusters: open — galaxies: individual — stars: abundances — stars: evolution
Record Number:CaltechAUTHORS:20190531-091632901
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190531-091632901
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95991
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:03 Jun 2019 21:30
Last Modified:03 Oct 2019 21:18

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