The Gould's Belt Very Large Array Survey II: The Serpens region

Abstract

We present deep ($\sim 17\mu$Jy) radio continuum observations of the Serpens molecular cloud, the Serpens south cluster, and the W40 region obtained using the Very Large Array in its A configuration. We detect a total of 146 sources, 29 of which are young stellar objects (YSOs), 2 are BV stars and 5 more are associated with phenomena related to YSOs. Based on their radio variability and spectral index, we propose that about 16 of the remaining 110 unclassified sources are also YSOs. For approximately 65% of the known YSOs detected here as radio sources, the emission is most likely non-thermal, and related to stellar coronal activity. As also recently observed in Ophiuchus, our sample of YSOs with X-ray counterparts lies below the fiducial Güdel & Benz relation. Finally, we analyze the proper motions of 9 sources in the W40 region. This allows us to better constrain the membership of the radio sources in the region.

Accepted in The Astrophysical Journal

References in corpus (9)

• Identifying the Low Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores
• The Spitzer Gould Belt Survey of Large Nearby Interstellar Clouds: Discovery of a Dense Embedded Cluster in the Serpens-Aquila Rift
• The Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey II: The First Four Epochs
• Statistical analyses of long-term variability of AGN at high radio frequencies
• CARMA Large Area Star Formation Survey: Observational Analysis of Filaments in the Serpens South Molecular Cloud
• Long-term radio variability of AGN: flare characteristics
• The onset of X-ray emission in young stellar objects: a Chandra observation of the Serpens star-forming region
• Searching for coronal radio emission from protostars using Very-Long-Baseline Interferometry
• Deep VLA Images of the HH 124 IRS Radio Cluster and its Surroundings and a New Determination of the Distance to NGC 2264

Cited by in corpus (15)

• The Gould's Belt Distances Survey (GOBELINS) I. Trigonometric parallax distances and depth of the Ophiuchus complex
• The Gould's Belt Distances Survey (GOBELINS) III. The distance to the Serpens/Aquila Molecular Complex
• Internal and relative motions of the Taurus and Ophiuchus star-forming regions
• The circumstellar environment around the embedded protostar EC 53
• The VLA Nascent Disk And Multiplicity Survey of Perseus Protostars (VANDAM). III. Extended Radio Emission from Protostars in Perseus
• Low Mass Stars as Tracers of Star and Cluster Formation
• Non-thermal radio continuum emission from young nearby stars
• ALMA Observations of SMM11 Reveal an Extremely Young Protostar in Serpens Main Cluster
• The distance to the Serpens South Cluster from H2O masers
• ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from its Exoplanet like a T Tauri Star from A Disk
• Discovery of 22 GHz Water Masers in the Serpens South Region
• HD 34736: An intensely magnetised double-lined spectroscopic binary with rapidly-rotating chemically peculiar B-type components
• The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio Luminosity$-$Spectral Type Dependence in Taurus$-$Auriga YSOs
• A Dual-Band Centimetre Continuum Monitoring Survey of Young Stellar Objects in the Coronet Cluster
• The population of compact radio sources in M 17