Triggered Star Formation from Bubbles S51, N68, and N131
Chuan-Peng Zhang, Jun-Jie Wang
TL;DR
This study examines the environments of three infrared dust bubbles to find evidence of star formation triggered by their expansion, contributing to understanding how such bubbles influence star formation processes.
Contribution
It provides new insights into the role of dust bubbles S51, N68, and N131 in triggering star formation, based on environmental analysis.
Findings
Evidence of triggered star formation around the bubbles
Identification of young stellar objects near the bubbles
Correlation between bubble expansion and star formation activity
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.
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