Beichman, C. A. (1986) Point Sources in the Orion Complex. In: Light on Dark Matter. Astrophysics and Space Science Library. No.124. Springer Netherlands , Dordrecht, pp. 279-292. ISBN 9789401085779. https://resolver.caltech.edu/CaltechAUTHORS:20200930-113054490
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Abstract
A 667 sq. deg. region in Orion contains thousands of IRAS sources, including stars, embedded sources, galaxies, as well as clumps in more extended emission (cirrus). Two particular types of sources, visible stars with infrared excesses characteristic of T Tauri stars and invisible, cool, embedded objects (L ~25 L_(sun)) are probably related to the formation of low mass stars in Orion.
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| Additional Information: | © D. Reidel Publishing Company 1986. The Infrared Astronomical Satellite was developed and operated by the Netherlands Agency for Aerospace Programs (NIVR), the US National Aeronautics and Space Administration (NASA) and the UK Science and Engineering Research Council (SERC). Thanks are due to R. Dumas for assistance in the preparation of this manuscript. The research described in this paper was performed by the Jet Propulsion Laboratory, under contract with NASA. | |||||||||
| Group: | Infrared Processing and Analysis Center (IPAC) | |||||||||
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| Series Name: | Astrophysics and Space Science Library | |||||||||
| Issue or Number: | 124 | |||||||||
| DOI: | 10.1007/978-94-009-4672-9_60 | |||||||||
| Record Number: | CaltechAUTHORS:20200930-113054490 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20200930-113054490 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 105676 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | George Porter | |||||||||
| Deposited On: | 30 Sep 2020 22:40 | |||||||||
| Last Modified: | 16 Nov 2021 18:45 |
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