Pillitteri, Ignazio and Wolk, S. J. and Megeath, S. T. and Allen, L. and Bally, J. and Gagné, Marc and Gutermuth, R. A. and Hartmann, L. and Micela, G. and Myers, P. and Oliveira, J. M. and Sciortino, S. and Walter, F. and Rebull, L. and Stauffer, J. (2014) Mapping the Star Formation in Orion A/L1641. In: The Labyrinth of Star Formation. Astrophysics and Space Science Proceedings. Vol.36. No.36. Springer , New York, NY, pp. 291-293. ISBN 978-3-319-03041-8. https://resolver.caltech.edu/CaltechAUTHORS:20170719-110502897
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Abstract
First phases of the process of star formation are characterized by excess in infrared and high X-ray emission. With Spitzer and XMM-Newton we have surveyed the Orion A part relative to the filamentary cloud Lynds 1641 (L1641). Furthermore, an extended spectroscopic survey has been realized to better constraint the cluster membership of stars without IR excess.
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| Additional Information: | © 2014 Springer. | ||||||||||||||||||||
| Series Name: | Astrophysics and Space Science Proceedings | ||||||||||||||||||||
| Issue or Number: | 36 | ||||||||||||||||||||
| Record Number: | CaltechAUTHORS:20170719-110502897 | ||||||||||||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20170719-110502897 | ||||||||||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||||||||||
| ID Code: | 79205 | ||||||||||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||||||||||
| Deposited By: | Ruth Sustaita | ||||||||||||||||||||
| Deposited On: | 19 Jul 2017 18:52 | ||||||||||||||||||||
| Last Modified: | 29 Apr 2020 22:05 |
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