SEDIGISM-ATLASGAL: Dense gas fraction and star formation efficiency across the Galactic disc
Artikel i vetenskaplig tidskrift, 2021

By combining two surveys covering a large fraction of the molecular material in the Galactic disc, we investigate the role spiral arms play in the star formation process. We have matched clumps identified by APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) with their parental giant molecular clouds (GMCs) as identified by SEDIGISM, and use these GMC masses, the bolometric luminosities, and integrated clump masses obtained in a concurrent paper to estimate the dense gas fractions (DGFgmc = ΣMclump/Mgmc) and the instantaneous star formation efficiencies (i.e. SFEgmc = ΣLclump/Mgmc). We find that the molecular material associated with ATLASGAL clumps is concentrated in the spiral arms (∼60 per cent found within ±10 km s-1 of an arm).We have searched for variations in the values of these physical parameters with respect to their proximity to the spiral arms, but find no evidence for any enhancement that might be attributable to the spiral arms. The combined results from a number of similar studies based on different surveys indicate that, while spiral-arm location plays a role in cloud formation and HI to H2 conversion, the subsequent star formation processes appear to depend more on local environment effects. This leads us to conclude that the enhanced star formation activity seen towards the spiral arms is the result of source crowding rather than the consequence of any physical process.

Galaxy: Kinematics and dynamics

Stars: Formation

Galaxy: Structure

Surveys

ISM: Clouds

Submillimetre: ISM

Författare

J. S. Urquhart

University Of Kent

C. Figura

Wartburg College

J. R. Cross

University Of Kent

M. Wells

University Of Kent

T. J.T. Moore

Liverpool John Moores University

D. J. Eden

Liverpool John Moores University

S. E. Ragan

Cardiff University

A. R. Pettitt

Hokkaido University

A. Duarte-Cabral

Cardiff University

D. Colombo

Max-Planck-Gesellschaft

F. Schuller

Max-Planck-Gesellschaft

Leibniz-Institut Für Astrophysik Potsdam

T. Csengeri

Université de Bordeaux

M. Mattern

Max-Planck-Gesellschaft

Université Paris-Saclay

H. Beuther

Max-Planck-Gesellschaft

K. M. Menten

Max-Planck-Gesellschaft

F. Wyrowski

Max-Planck-Gesellschaft

L. D. Anderson

West Virginia University

P. J. Barnes

Space Science Institute

M. Beltrán

Osservatorio Astrofisico di Arcetri

S. J. Billington

University Of Kent

Leonardo Bronfman

Universidad de Chile (UCH)

A. Giannetti

Istituto di Radioastronomia

Jouni Kainulainen

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Galaktisk astrofysik

J. Kauffmann

Massachusetts Institute of Technology (MIT)

M. Y. Lee

Korea Astronomy and Space Science Institute

S. Leurini

INAF Osservatorio Astronomico di Cagliari

S. N.X. Medina

Max-Planck-Gesellschaft

F.M. Montenegro-Montes

European Southern Observatory Santiago

Manuel Riener

Max-Planck-Gesellschaft

Andrew Rigby

Cardiff University

A. Sanchez-Monge

Universität zu Köln

P. Schilke

Universität zu Köln

E. Schisano

Istituto nazionale di astrofisica (INAF)

A. Traficante

Istituto nazionale di astrofisica (INAF)

M. Wienen

University of Exeter

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 500 3 3050-3063

Ämneskategorier

Astronomi, astrofysik och kosmologi

Kemiska processer

Annan kemi

DOI

10.1093/mnras/staa2512

Mer information

Senast uppdaterat

2021-07-08