The Gould's belt very large array survey. III. the orion region

dc.contributorKounkel, M., Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, United States; Hartmann, L., Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, United States; Loinard, L., Centro de Radiostronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, México, Max Planck Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany; Mioduszewski, A.J., National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, NM 87801, United States; Dzib, S.A., Max Planck Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany; Ortiz-León, G.N., Centro de Radiostronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, México; Rodríguez, L.F., Centro de Radiostronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, México; Pech, G., Centro de Radiostronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, México; Rivera, J.L., Centro de Radiostronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia 58089, México; Torres, R.M., Instituto de Astronomía y Meteorología, Universidad de Guadalajara, Avenida Vallarta No. 2602, Col. Arcos Vallarta, CP 44130, Guadalajara, Jalisco, México; Boden, A.F., Division of Physics, Math and Astronomy, California Institute of Technology, 1200 E California Blvd., Pasadena, CA 91125, United States; Evans, N.J., Department of Astronomy, University of Texas at Austin, 1 University Station, C1400, Austin, TX 78712, United States; Briceño, C., Cerro Tololo Interamerican Observatory, Casilla 603, La-Serena, Chile; Tobin, J., National Radio Astronomy Observatory, Charlottesville, VA 22903, United States
dc.creatorKounkel, M.
dc.creatorHartmann, L.
dc.creatorLoinard, L.
dc.creatorMioduszewski, A.J.
dc.creatorDzib, S.A.
dc.creatorOrtiz-Leon, G.N.
dc.creatorRodriguez, L.F.
dc.creatorPech, G.
dc.creatorRivera, J.L.
dc.creatorTorres, R.M.
dc.creatorBoden, A.F.
dc.creatorEvans, N.J.
dc.creatorBriceno, C.
dc.creatorTobin, J.
dc.date.accessioned2015-09-15T19:08:24Z
dc.date.accessioned2022-11-02T15:19:53Z
dc.date.available2015-09-15T19:08:24Z
dc.date.available2022-11-02T15:19:53Z
dc.date.created2015-09-15T19:08:24Z
dc.date.issued2014
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84904187363&partnerID=40&md5=d3315693e9e8a062479995447ad844ca
dc.identifierhttp://hdl.handle.net/20.500.12104/45163
dc.identifier10.1088/0004-637X/790/1/49
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5012456
dc.description.abstractWe present results from a high-sensitivity (60 ?Jy), large-scale (2.26 deg2) 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. © 2014. The American Astronomical Society. All rights reserved..
dc.relationScopus
dc.relationWOS
dc.relationAstrophysical Journal
dc.relation790
dc.relation1
dc.titleThe Gould's belt very large array survey. III. the orion region
dc.typeArticle


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