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Infrared Studies of Star Formation

Werner, M. W. and Becklin, E. E. and Neugebauer, G. (1977) Infrared Studies of Star Formation. Science, 197 (4305). pp. 723-732. ISSN 0036-8075. http://resolver.caltech.edu/CaltechAUTHORS:20151117-080411276

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Abstract

The lifetime of a massive star before it begins to deplete its nuclear fuel is less than 5 million years (1). In contrast, the age of the galaxy is more than 10 billion years (2); nevertheless, many massive and short-lived stars have been identified by observations at optical wavelengths. These massive stars must have formed very recently relative to the age of the galaxy, and therefore star formation must be occurring in the galaxy at the present time.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.197.4305.723DOIArticle
http://www.sciencemag.org/content/197/4305/723.extractPublisherArticle
http://www.jstor.org/stable/1744843JSTORArticle
Additional Information:© 1977 American Association for the Advancement of Science. This work was supported by NASA grants NGR 5-002-281 and NGL 5-002-207 and by NSF grant MPS 74-18555AOI. M.W.W. is an Alfred P. Sloan Foundation Fellow. We thank many colleagues, especially I. Gatley, A. E. Glassgold, J. R. Houck, R. B. Leighton, G. H. Rieke, C. G. Wynn-Williams, and G. Zweig, for their comments on the manuscript.
Funders:
Funding AgencyGrant Number
NASANGR 5-002-281
NASANGL 5-002-207
NSFMPS 74-18555A01
Alfred P. Sloan FoundationUNSPECIFIED
Record Number:CaltechAUTHORS:20151117-080411276
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20151117-080411276
Official Citation:Infrared Studies of Star Formation M. W. Werner, E. E. Becklin, and G. Neugebauer Science 19 August 1977: 197 (4305), 723-732. [DOI:10.1126/science.197.4305.723]
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:62147
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:17 Nov 2015 18:40
Last Modified:13 Feb 2019 18:06

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