Triggered Star Formation from Bubbles S51, N68, and N131

Abstract

We investigated the environment of the infrared dust bubbles S51, N68, and N131 from catalogue of Churchwell et al. (2006), and searched for evidence of triggered star formation.

arXiv commentProceedings IAU Symposium No. 292, 2012

References in corpus (1)

• Molecular line mapping of the giant molecular cloud associated with RCW 106 - III. Multi-molecular line mapping