Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. ATLASGAL -- Evolutionary trends in high-mass star formation
 

ATLASGAL -- Evolutionary trends in high-mass star formation

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2022
Author(s)
Urquhart, J. S.
•
Wells, M. R. A.
•
Pillai, T.
•
Leurini, Silvia  
•
Giannetti, A.  
•
Moore, T. J. T.
•
Thompson, M. A.
•
Figura, C.
•
Colombo, D.
•
Yang, A. Y.
•
Koenig, C.
•
Wyrowski, F.
•
Menten, K. M.
•
Rigby, A. J.
•
Eden, D. J.
•
Ragan, S. E.
DOI
10.1093/mnras/stab3511
Abstract
ATLASGAL is a 870-mircon dust survey of 420 square degrees of the inner Galactic plane and has been used to identify ~10 000 dense molecular clumps. Dedicated follow-up observations and complementary surveys are used to characterise the physical properties of these clumps, map their Galactic distribution and investigate the evolutionary sequence for high-mass star formation. The analysis of the ATLASGAL data is ongoing: we present an up-to-date version of the catalogue. We have classified 5007 clumps into four evolutionary stages (quiescent, protostellar, young stellar objects and HII regions) and find similar numbers of clumps in each stage, suggesting a similar lifetime. The luminosity-to-mass (L/M) ratio curve shows a smooth distribution with no significant kinks or discontinuities when compared to the mean values for evolutionary stages indicating that the star-formation process is continuous and that the observational stages do not represent fundamentally different stages or changes in the physical mechanisms involved. We compare the evolutionary sample with other star-formation tracers (methanol and water masers, extended green objects and molecular outflows) and find that the association rates with these increases as a function of evolutionary stage, confirming that our classification is reliable. This also reveals a high association rate between quiescent sources and molecular outflows, revealing that outflows are the earliest indication that star formation has begun and that star formation is already ongoing in many of the clumps that are dark even at 70 micron.
Volume
510
Issue
3
Start page
3389
Uri
http://hdl.handle.net/20.500.12386/32650
Url
http://arxiv.org/abs/2111.12816v2
https://academic.oup.com/mnras/article-abstract/510/3/3389/6449386?redirectedFrom=fulltext&login=false
Issn Identifier
0035-8711
Ads BibCode
2022MNRAS.510.3389U
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

2111.12816.pdf

Description
postprint
Size

2.37 MB

Format

Adobe PDF

Checksum (MD5)

af3e6216eb9e7609c7b313df4078d765

Loading...
Thumbnail Image
Name

stab3511.pdf

Description
PDF editoriale
Size

3.78 MB

Format

Adobe PDF

Checksum (MD5)

a9c7ea4b26485b3e29a95d2175240869

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback