Triggered Star Formation from Bubbles S51, N68, and N131
Abstract
We investigated the environment of the infrared dust bubbles S51 (Zhang & Wang 2012a), N68 (Zhang & Wang 2012b), and N131 (Zhang et al. 2012) from catalogue of Churchwell et al. (2006), and searched for evidence of triggered star formation.
- Publication:
-
Molecular Gas, Dust, and Star Formation in Galaxies
- Pub Date:
- March 2013
- DOI:
- 10.1017/S1743921313000458
- arXiv:
- arXiv:1209.3176
- Bibcode:
- 2013IAUS..292...65Z
- Keywords:
-
- infrared: stars;
- stars: formation;
- ISM: bubbles;
- HII regions;
- Astrophysics - Astrophysics of Galaxies;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- Proceedings IAU Symposium No. 292, 2012