作者: Thomas J. Haworth , Tim J. Harries , David M. Acreman , David A. Rundle
DOI: 10.1093/MNRAS/STT427
关键词: Capital (economics) 、 Physics 、 Methods observational 、 Star formation 、 Astrophysics 、 Molecular line 、 Dirac (software) 、 Astronomy
摘要: The calculations presented here were performed using the University of Exeter Supercomputer, part DiRAC Facility jointly funded by STFC, Large Facilities Capital Fund BIS and Exeter. TJH is an STFC studentship. We thank Chris Brunt, Emily Drabek Jennifer Hatchell for useful discussions. also referee their comments, which helped to improve paper.