dc.contributor.author | Forbrich, Jan | |
dc.contributor.author | Rivilla, Victor M. | |
dc.contributor.author | Menten, Karl M. | |
dc.contributor.author | Reid, Mark J. | |
dc.contributor.author | Chandler, Claire J. | |
dc.contributor.author | Rau, Urvashi | |
dc.contributor.author | Bhatnagar, Sanjay | |
dc.contributor.author | Wolk, Scott J. | |
dc.contributor.author | Meingast, Stefan | |
dc.date.accessioned | 2017-06-22T16:34:34Z | |
dc.date.available | 2017-06-22T16:34:34Z | |
dc.date.issued | 2016-05-10 | |
dc.identifier.citation | Forbrich , 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.issn | 0004-637X | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1603.05666v1 | |
dc.identifier.other | ORCID: /0000-0001-8694-4966/work/62751198 | |
dc.identifier.uri | http://hdl.handle.net/2299/18475 | |
dc.description | This 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.abstract | We 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.extent | 1922065 | |
dc.language.iso | eng | |
dc.relation.ispartof | The Astrophysical Journal | |
dc.subject | astro-ph.SR | |
dc.subject | astro-ph.GA | |
dc.title | The Population of Compact Radio Sources in the Orion Nebula Cluster | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.3847/0004-637X/822/2/93 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |