We present results from a high-sensitivity (60 μJy), large-scale (2.26 deg2) survey obtained with the Karl G. Jansky Very Large Array as part of the Gould's Belt Survey program. We detected 374 and 354 sources at 4.5 and 7.5 GHz, respectively. Of these, 148 are associated with previously known young stellar objects (YSOs). Another 86 sources previously unclassified at either optical or infrared wavelengths exhibit radio properties that are consistent with those of young stars. The overall properties of our sources at radio wavelengths such as their variability and radio to X-ray luminosity relation are consistent with previous results from the Gould's Belt Survey. Our detections provide target lists for follow-up Very Long Baseline Array ra...
Funding Information: We thank the anonymous referee for helpful and constructive comments that lead ...
V. M. Rivilla, et al., “Short- and Long-term Radio Variability of Young Stars in the Orion Nebula Cl...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using HARP (Heterodyne Arr...
We present results from a high-sensitivity (60 ?Jy), large-scale (2.26 deg2) survey obtained with th...
We present results from a high-sensitivity (60 mu Jy), large-scale (2.26 deg(2)) survey obtained wit...
We present large-scale ( ∼ 2000 square arcminutes), deep ( ∼ 20 µJy), high-resolution ( ∼ 1′′) radio...
We present large-scale (similar to 2000 arcmin(2)), deep (similar to 20 mu Jy), high-resolution (sim...
We present deep (similar to 17 mu Jy) radio continuum observations of the Serpens molecular cloud, t...
International audienceWe present the results of the Gould’s Belt Distances Survey of young star-form...
We present a multi-epoch radio study of the Taurus-Auriga star-forming complex made with the Karl G....
Context. The recent star formation history in the solar vicinity is not yet well constrained, and th...
We present Karl G. Jansky Very Large Array 1.3, 3.6, and 6 cm continuum maps of compact radio source...
We report first results on the large-scale distribution of the ROSAT All-Sky Survey (RASS) X-ray sou...
A survey for radio emission at 6 GHz and 9 GHz toward three regions of massive star formation in the...
In recent years, high-energy processes in young stellar objects have largely been studied using X-ra...
Funding Information: We thank the anonymous referee for helpful and constructive comments that lead ...
V. M. Rivilla, et al., “Short- and Long-term Radio Variability of Young Stars in the Orion Nebula Cl...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using HARP (Heterodyne Arr...
We present results from a high-sensitivity (60 ?Jy), large-scale (2.26 deg2) survey obtained with th...
We present results from a high-sensitivity (60 mu Jy), large-scale (2.26 deg(2)) survey obtained wit...
We present large-scale ( ∼ 2000 square arcminutes), deep ( ∼ 20 µJy), high-resolution ( ∼ 1′′) radio...
We present large-scale (similar to 2000 arcmin(2)), deep (similar to 20 mu Jy), high-resolution (sim...
We present deep (similar to 17 mu Jy) radio continuum observations of the Serpens molecular cloud, t...
International audienceWe present the results of the Gould’s Belt Distances Survey of young star-form...
We present a multi-epoch radio study of the Taurus-Auriga star-forming complex made with the Karl G....
Context. The recent star formation history in the solar vicinity is not yet well constrained, and th...
We present Karl G. Jansky Very Large Array 1.3, 3.6, and 6 cm continuum maps of compact radio source...
We report first results on the large-scale distribution of the ROSAT All-Sky Survey (RASS) X-ray sou...
A survey for radio emission at 6 GHz and 9 GHz toward three regions of massive star formation in the...
In recent years, high-energy processes in young stellar objects have largely been studied using X-ra...
Funding Information: We thank the anonymous referee for helpful and constructive comments that lead ...
V. M. Rivilla, et al., “Short- and Long-term Radio Variability of Young Stars in the Orion Nebula Cl...
The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using HARP (Heterodyne Arr...