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High-mass Star Formation towards the southern infrared Bubble S10

Vig, S.; Ghosh, S. K.; Ishwara-Chandra, C. H. +2 more

We present a multi-wavelength analysis of the southern infrared bubble S10. Radio continuum emission is detected towards the bubble at 610 and 1280 MHz, and the bubble is estimated to be powered by massive stars of spectral type B0.5 - B0. A Class I/II type source, with an estimated mass of 6.2 Msol, lies 7'' from the radio peak. Six massive clump…