arXiv Analytics

Sign in

arXiv:1603.05666 [astro-ph.SR]AbstractReferencesReviewsResources

The Population of Compact Radio Sources in the Orion Nebula Cluster

Jan Forbrich, Victor M. Rivilla, Karl M. Menten, Mark J. Reid, Claire J. Chandler, Urvashi Rau, Sanjay Bhatnagar, Scott J. Wolk, Stefan Meingast

Published 2016-03-17Version 1

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.

Related articles: Most relevant | Search more
arXiv:1206.5339 [astro-ph.SR] (Published 2012-06-22)
Compact radio sources in M17
arXiv:2402.12258 [astro-ph.SR] (Published 2024-02-19, updated 2025-01-13)
Low-mass Runaways from the Orion Nebula Cluster -- Kinematic Age Constraints on Star Cluster Formation
arXiv:2403.07083 [astro-ph.SR] (Published 2024-03-11)
HST Survey of the Orion Nebula Cluster in ACS/Visible and WFC3/IR Bands. IV. A Bayesian multicolor study of stellar parameters in the ONC