The Population of Compact Radio Sources in the Orion Nebula Cluster

Jan Forbrich, V. M. Rivilla, Karl M. Menten, Mark J. Reid, C. J. Chandler, Stefan Meingast

Publications: Contribution to journalArticlePeer Reviewed

Abstract

We present a deep centimeter-wavelength catalog of the Orion Nebula Cluster (ONC), based on a 30 hr 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 and 7.3 GHz. A total of 556 compact sources were detected in a map with a nominal rms noise of 3 μJy bm-1, 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.
Original languageEnglish
Article number93
Number of pages13
JournalThe Astrophysical Journal
Volume822
Issue number2
DOIs
Publication statusPublished - May 2016

Austrian Fields of Science 2012

  • 103003 Astronomy
  • 103004 Astrophysics

Keywords

  • EMISSION
  • SOLAR
  • STARS
  • VARIABILITY
  • X-RAY
  • X-rays: stars
  • YOUNG STELLAR OBJECTS
  • radio continuum: stars
  • stars: coronae
  • stars: formation

Fingerprint

Dive into the research topics of 'The Population of Compact Radio Sources in the Orion Nebula Cluster'. Together they form a unique fingerprint.

Cite this