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dc.contributor.authorForbrich, Jan
dc.contributor.authorRivilla, Victor M.
dc.contributor.authorMenten, Karl M.
dc.contributor.authorReid, Mark J.
dc.contributor.authorChandler, Claire J.
dc.contributor.authorRau, Urvashi
dc.contributor.authorBhatnagar, Sanjay
dc.contributor.authorWolk, Scott J.
dc.contributor.authorMeingast, Stefan
dc.date.accessioned2017-06-22T16:34:34Z
dc.date.available2017-06-22T16:34:34Z
dc.date.issued2016-05-10
dc.identifier.citationForbrich , J , Rivilla , V M , Menten , K M , Reid , M J , Chandler , C J , Rau , U , Bhatnagar , S , Wolk , S J & Meingast , S 2016 , ' The Population of Compact Radio Sources in the Orion Nebula Cluster ' , The Astrophysical Journal , vol. 822 , no. 2 . https://doi.org/10.3847/0004-637X/822/2/93
dc.identifier.issn0004-637X
dc.identifier.otherArXiv: http://arxiv.org/abs/1603.05666v1
dc.identifier.otherORCID: /0000-0001-8694-4966/work/62751198
dc.identifier.urihttp://hdl.handle.net/2299/18475
dc.descriptionThis document is the Accepted Manuscript version of the following article: J. Forbrich, et al, ‘The population of compact radio sources in the Orion Nebula Cluster’, The Astrophysical Journal, Vol. 822 (2), May 2016. The Version of Record is available online at DOI: HTTPS://DOI.ORG/10.3847/0004-637x/822/2/93. © 2016. The American Astronomical Society. All rights reserved.
dc.description.abstractWe present a deep centimeter-wavelength catalog of the Orion Nebula Cluster (ONC), based on a 30h single-pointing observation with the Karl G. Jansky Very Large Array in its high-resolution A-configuration using two 1 GHz bands centered at 4.7 GHz and 7.3 GHz. A total of 556 compact sources were detected in a map with a nominal rms noise of 3 muJy/bm, limited by complex source structure and the primary beam response. Compared to previous catalogs, our detections increase the sample of known compact radio sources in the ONC by more than a factor of seven. The new data show complex emission on a wide range of spatial scales. Following a preliminary correction for the wideband primary-beam response, we determine radio spectral indices for 170 sources whose index uncertainties are less than +/-0.5. We compare the radio to the X-ray and near-infrared point-source populations, noting similarities and differences.en
dc.format.extent1922065
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.subjectastro-ph.SR
dc.subjectastro-ph.GA
dc.titleThe Population of Compact Radio Sources in the Orion Nebula Clusteren
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.3847/0004-637X/822/2/93
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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