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The Gould's Belt Very Large Array Survey. III. The Orion Region

Kounkel, Marina and Hartmann, Lee and Loinard, Laurent and Mioduszewski, Amy J. and Dzib, Sergio A. and Ortiz-Leόn, Gisela N. and Rodríguez, Luis F. and Pech, Gerardo and Rivera, Juana L. and Torres, Rosa M. and Boden, Andrew F. and Evans, Neal J., II and Briceño, Cesar and Tobin, John J. (2014) The Gould's Belt Very Large Array Survey. III. The Orion Region. Astrophysical Journal, 790 (1). Art. No. 49. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20140818-091950805

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Abstract

We present results from a high-sensitivity (60 μJy), large-scale (2.26 deg^2) survey obtained with the Karl G. Jansky Very Large Array as part of the Gould's Belt Survey program. We detected 374 and 354 sources at 4.5 and 7.5 GHz, respectively. Of these, 148 are associated with previously known young stellar objects (YSOs). Another 86 sources previously unclassified at either optical or infrared wavelengths exhibit radio properties that are consistent with those of young stars. The overall properties of our sources at radio wavelengths such as their variability and radio to X-ray luminosity relation are consistent with previous results from the Gould's Belt Survey. Our detections provide target lists for follow-up Very Long Baseline Array radio observations to determine their distances as YSOs are located in regions of high nebulosity and extinction, making it difficult to measure optical parallaxes.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/790/1/49DOIArticle
http://iopscience.iop.org/0004-637X/790/1/49/articlePublisherArticle
http://arxiv.org/abs/1406.1809arXivDiscussion Paper
ORCID:
AuthorORCID
Hartmann, Lee0000-0003-1430-8519
Tobin, John J.0000-0002-6195-0152
Additional Information:© 2014 The American Astronomical Society. Received 14 April 2014, accepted for publication 6 June 2014 Published 2 July 2014. This work was supported in part by the University of Michigan. L.L. is grateful to the von Humboldt Stiftung for financial support. L.L., S.D., L.F.R., G.N.O., G.P., and J.L.R. acknowledge the financial support of DGAPA, UNAM, and CONACyT, México. J.T. acknowledges support provided by NASA through Hubble Fellowship grant #HST-HF-51300.01-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. AIPS is produced and maintained by the National Radio Astronomy Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This research has made use of the SIMBAD database and VizieR catalogue access tool, operated at CDS, Strasbourg, France.
Funders:
Funding AgencyGrant Number
University of MichiganUNSPECIFIED
Alexander von Humboldt FoundationUNSPECIFIED
DGAPAUNSPECIFIED
UNAMUNSPECIFIED
CONACyTUNSPECIFIED
NASA Hubble FellowshipHST-HF-51300.01-A
Subject Keywords:astrometry; magnetic fields; radiation mechanisms: non-thermal; radio continuum: stars; techniques: interferometric
Record Number:CaltechAUTHORS:20140818-091950805
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140818-091950805
Official Citation:The Gould's Belt Very Large Array Survey. III. The Orion Region Marina Kounkel et al. 2014 ApJ 790 49
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:48643
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:19 Aug 2014 21:52
Last Modified:26 May 2017 18:17

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