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Mapping the Star Formation in Orion A/L1641

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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-3-319-03041-8_56DOIArticle
http://rdcu.be/ujCTPublisherFree ReadCube access
ORCID:
AuthorORCID
Wolk, S. J.0000-0002-0826-9261
Megeath, S. T.0000-0001-7629-3573
Bally, J.0000-0001-8135-6612
Gutermuth, R. A.0000-0002-6447-899X
Hartmann, L.0000-0003-1430-8519
Micela, G.0000-0002-9900-4751
Walter, F.0000-0003-4793-7880
Rebull, L.0000-0001-6381-515X
Stauffer, J.0000-0003-3595-7382
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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