Surveys of molecular gas in the Solar neighbourhood and the inner Galaxy have shown that molecular clouds are statistically equilibrium between the turbulent kinetic energy (E_k) and the self-gravitational energy (E_g), namely the virial parameter alpha_vir=2E_k/|E_g|~1. However, our recent work shows that alpha_vir decreases towards the metal-poor outer Galaxy and is systematically smaller than unity at Galactocentric radii Rgc > 15 kpc. This suggests that turbulence is insufficient to support against the cloud's self-gravity in such conditions. Nevertheless, the current data can not resolve the detailed cloud structure, leading to uncertainties in estimating |E_g| and inability to decompose the possible substructures. Therefore, we propose GBT/Argus observations towards seven clouds at Rgc > 15 kpc, targeting the 13CO J=1-0 line. With a ~0.5 pc resolution, the morphology and the velocity fields are key to understanding the low virial parameters and possible star formation activities in metal-poor molecular clouds from the outer disk of the Milky Way.
Name | Institution |
---|---|
Lingrui Lin * | Nanjing University |
Gan Luo | Institut de Radio Astronomique Millimétrique |
Zhiyu zhang | Nanjing University |
Junzhi Wang | Purple Mountain Observatory, CAS; Shanghai Astronomical Observatory, CAS; Nanjing University; Guangxi University |
Yichen Sun | Nanjing University |
Di Li | National Astronomical Observatories, CAS; Space Science Institute |
Jialu Li | Maryland, University of |
Siyi Feng | Max-Planck-Institut für extraterrestrische Physik; Max-Planck-Institut für Astronomie; National Astronomical Observatory of Japan ; Xiamen University; East Asian Observatory |
Hauyu Liu | Academia Sinica; European Southern Observatory; National Sun Yat-sen University |
yan sun | Purple Mountain Observatory, CAS |
Yong Shi | Nanjing University |
Yan Gong | Max-Planck-Institut für Radioastronomie; Purple Mountain Observatory, CAS |
Thomas Bisbas | Köln, Universität zu |
* indicates the PI