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 language | English |
---|---|
Article number | 93 |
Number of pages | 13 |
Journal | The Astrophysical Journal |
Volume | 822 |
Issue number | 2 |
DOIs | |
Publication status | Published - 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