The Gould's Belt Very Large Array Survey. IV. The Taurus-Auriga Complex

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dc.contributor.utaustinauthorEvans, Neal J.en_US
dc.creatorDzib, Sergio A.en_US
dc.creatorLoinard, Laurenten_US
dc.creatorRodriguez, Luis F.en_US
dc.creatorMioduszewski, Amy J.en_US
dc.creatorOrtiz-Leon, Gisela N.en_US
dc.creatorKounkel, Marina A.en_US
dc.creatorPech, Gerardoen_US
dc.creatorRivera, Juana L.en_US
dc.creatorTorres, Rosa M.en_US
dc.creatorBoden, Andrew F.en_US
dc.creatorHartmann, Leeen_US
dc.creatorEvans, Neal J.en_US
dc.creatorBriceno, Cesaren_US
dc.creatorTobin, Johnen_US
dc.date.accessioned2016-04-28T19:38:10Z
dc.date.available2016-04-28T19:38:10Z
dc.date.issued2015-03en
dc.description.abstractWe present a multi-epoch radio study of the Taurus-Auriga star-forming complex made with the Karl G. Jansky Very Large Array at frequencies of 4.5 GHz and 7.5 GHz. We detect a total of 610 sources, 59 of which are related to young stellar objects (YSOs) and 18 to field stars. The properties of 56% of the young stars are compatible with non-thermal radio emission. We also show that the radio emission of more evolved YSOs tends to be more non-thermal in origin and, in general, that their radio properties are compatible with those found in other star-forming regions. By comparing our results with previously reported X-ray observations, we notice that YSOs in Taurus-Auriga follow a Giidel Benz relation with k = 0.03, as we previously suggested for other regions of star formation. In general, YSOs in Taurus-Auriga and in all the previous studied regions seem to follow this relation with a dispersion of similar to 1 dex. Finally, we propose that most of the remaining sources are related with extragalactic objects but provide a list of 46 unidentified radio sources whose radio properties are compatible with a YSO nature.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipNational Radio Astronomical Observatory (NRAO)en_US
dc.description.sponsorshipEuropean Southern Observatory (ESO)en_US
dc.description.sponsorshipNational Astronomical Observatory of Japan (NAOJ)en_US
dc.description.sponsorshipCSIRO Australia Telescope National Facility (CSIRO/ATNF)en_US
dc.description.sponsorshipNetherlands Institute for Radio Astronomy (ASTRON)en_US
dc.identifierdoi:10.15781/T2DZ5B
dc.identifier.Filename2015_03_gouldsbeltiv.pdfen_US
dc.identifier.citationDzib, Sergio A., Laurent Loinard, Luis F. Rodr�guez, Amy J. Mioduszewski, Gisela N. Ortiz-Le�n, Marina A. Kounkel, Gerardo Pech et al. "The Gould's Belt Very Large Array Survey. IV. The Taurus-Auriga Complex." The Astrophysical Journal, Vol. 801, No. 2 (Mar., 2015): 91.en_US
dc.identifier.doi10.1088/0004-637x/801/2/91en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/2152/34978
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journalen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectradio continuum: starsen_US
dc.subjectradiation mechanisms: non-thermalen_US
dc.subjectradiationen_US
dc.subjectmechanisms: thermalen_US
dc.subjecttechniques: interferometricen_US
dc.subjectherbig-ae/be starsen_US
dc.subjectx-ray-emissionen_US
dc.subjectbase-line interferometryen_US
dc.subjectradio-continuum emissionen_US
dc.subjectyoung stellar objectsen_US
dc.subjectharo energy-sourcesen_US
dc.subjectt-taurien_US
dc.subjectvlba determinationen_US
dc.subjectexciting sourcesen_US
dc.subjectforming regionsen_US
dc.subjectastronomy & astrophysicsen_US
dc.titleThe Gould's Belt Very Large Array Survey. IV. The Taurus-Auriga Complexen_US
dc.typeArticleen_US

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