AMI Large Array radio continuum observations of Spitzer c2d small clouds and cores
arXiv:1009.0348 · doi:10.1111/j.1365-2966.2010.17644.x
Abstract
We perform deep 1.8 cm radio continuum imaging towards thirteen protostellar regions selected from the Spitzer c2d small clouds and cores programme at high resolution (25") in order to detect and quantify the cm-wave emission from deeply embedded young protostars. Within these regions we detect fifteen compact radio sources which we identify as radio protostars including two probable new detections. The sample is in general of low bolometric luminosity and contains several of the newly detected VeLLO sources. We determine the 1.8 cm radio luminosity to bolometric luminosity correlation, L_rad -L_bol, for the sample and discuss the nature of the radio emission in terms of the available sources of ionized gas. We also investigate the L_rad-L_IR correlation and suggest that radio flux density may be used as a proxy for the internal luminosity of low luminosity protostars.
submitted MNRAS
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Cited by in corpus (9)
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- The VLA Nascent Disk And Multiplicity Survey of Perseus Protostars (VANDAM). III. Extended Radio Emission from Protostars in Perseus
- AMI radio continuum observations of young stellar objects with known outflows
- Radio continuum observations of Class I protostellar disks in Taurus: constraining the greybody tail at centimetre wavelengths
- Radio Properties of Young Stellar Objects in the Core of the Serpens South Infrared Dark Cloud
- AMI-LA radio continuum observations of Spitzer c2d small clouds and cores: Serpens region
- CARMA Observations of Galactic Cold Cores: Searching for Spinning Dust Emission