The Population of Compact Radio Sources in the Orion Nebula Cluster
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.
Item Type | Article |
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Additional information | 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. |
Keywords | astro-ph.sr, astro-ph.ga |
Date Deposited | 15 May 2025 13:26 |
Last Modified | 31 May 2025 00:10 |