W49A: A starburst triggered by expanding shells
T.-C. Peng, F. Wyrowski, F. F. S. van der Tak, K. M. Menten, and C. M., Walmsley

TL;DR
This study reveals that expanding shells driven by massive stars in W49A likely triggered the intense starburst activity in this giant molecular cloud, supported by multi-scale infrared and CO observations.
Contribution
It provides new evidence linking expanding shells and gas ejections to starburst triggering in W49A through detailed multi-scale molecular line analysis.
Findings
Identified two expanding shells with a mass of ~1.9 x 10^4 M_sun.
Estimated shell expansion speed of ~5 km/s and age of 0.3-0.7 million years.
Detected gas ejections with energies of a few times 10^50 erg.
Abstract
W49A is a giant molecular cloud which harbors some of the most luminous embedded clusters in the Galaxy. However, the explanation for this starburst-like phenomenon is still under debate. Methods. We investigated large-scale Spitzer mid-infrared images together with a Galatic Ring Survey 13CO J = 1-0 image, complemented with higher resolution (~ 11 arcsec) 13CO J = 2-1 and C18O J = 2-1 images over a ~ 15 x 13 pc^2 field obtained with the IRAM 30m telescope. Two expanding shells have been identified in the mid-infrared images, and confirmed in the position-velocity diagrams made from the 13CO J = 2-1 and C18O J = 2-1 data. The mass of the averaged expanding shell, which has an inner radius of ~ 3.3 pc and a thickness of ~ 0.41 pc, is about 1.9 x 10^4 M*. The total kinetic energy of the expanding shells is estimated to be ~ 10^49 erg which is probably provided by a few massive stars,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
