SQ-A: A Collision Triggered Starburst in Intra-Group Medium of Stephan's Quintet
C. K. Xu, C. Cheng, M. S. Yun, P. N. Appleton, B. H. C. Emonts, J. Braine, S. C. Gallagher, P. Guillard, U. Lisenfeld, E. OSullivan, F. Renaud, P. Aromal, P.-A. Duc, A. Labiano, A. Togi

TL;DR
This study provides observational evidence that a starburst in Stephan's Quintet's intra-group medium is triggered by a high-speed collision between gas systems, leading to diverse star formation activities.
Contribution
It offers new high-resolution ALMA and VLA data showing gas interactions and their role in starburst triggering in Stephan's Quintet.
Findings
Gas bridging between systems indicates cloud-cloud collision.
Star formation varies significantly among different gas kinematic systems.
Gas compression enhances star formation, while vortices suppress it.
Abstract
We present new observational evidence supporting the hypothesis that SQ-A, a starburst in the intra-group medium (IGrM) of Stephan's Quintet (SQ), is triggered by a high-speed collision between two gas systems, one associated with the IGrM (v~6900 km/s) and another with the intruder galaxy NGC7318b (v~6000 km/s). The new ALMA CO(2-1) dataset has angular resolutions between 0.2" and 7.0" and the new VLA HI datacube an angular resolution of 6.6" * 7.9". The CO maps show that the two gas systems are bridged by another system with an intermediate velocity of ~6600 km/s, whereas the HI data show that the component of v~6600 km/s fits well into a gap in the more extended v~6000 km/s component, albeit with a displacement of ~5 kpc. Both the bridge and the complementary distributions between different gas systems are common features of starbursts triggered by cloud-cloud collision. An analysis…
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