From a survey of 729 cores based on JCMT/SCUBA data, we present an analysis of 17 candidate starless cores with masses that exceed their stable Jeans masses. We re-examine the classification of these super-Jeans cores using Spitzer maps and find that 3 are re-classified as protostellar, 11 have ambiguous emission near the core positions, and 3 appear to be genuinely starless. We suggest that the 3 starless and 11 undetermined super-Jeans cores represent excellent targets for future observational and computational study to understand the evolution of dense cores and the process of star formation. © 2010. The American Astronomical Society.
CITATION STYLE
Sadavoy, S. I., Di Francesco, J., & Johnstone, D. (2010). Starless super-jeans cores in four Gould belt clouds. Astrophysical Journal Letters, 718(1 PART 2). https://doi.org/10.1088/2041-8205/718/1/L32
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