The Open UniversitySkip to content
 

Herschelobservations of the W3 GMC (II): clues to the formation of clusters of high-mass stars

Rivera-Ingraham, A.; Martin, P. G.; Polychroni, D.; Schneider, N.; Motte, F.; Bontemps, S.; Hennemann, M.; Men'shchikov, A.; Luong, Q. Nguyen; Zavagno, A.; André, Ph.; Bernard, J.-Ph.; Francesco, J. Di; Fallscheer, C.; Hill, T.; Könyves, V.; Marston, A.; Pezzuto, S.; Rygl, K. L. J.; Spinoglio, L. and White, G. J. (2015). Herschelobservations of the W3 GMC (II): clues to the formation of clusters of high-mass stars. The Astrophysical Journal, 809(1), article no. 81.

Full text available as:
[img]
Preview
PDF (Accepted Manuscript) - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (380kB) | Preview
DOI (Digital Object Identifier) Link: https://doi.org/10.1088/0004-637X/809/1/81
Google Scholar: Look up in Google Scholar

Abstract

The W3 giant molecular cloud is a prime target for investigating the formation of high-mass stars and clusters. This second study of W3 within the HOBYS Key Program provides a comparative analysis of subfields within W3 to further constrain the processes leading to the observed structures and stellar population. Probability density functions (PDFs) and cumulative mass distributions (CMDs) were created from dust column density maps, quantified as extinction AV. The shape of the PDF, typically represented with a lognormal function at low Av “breaking” to a power-law tail at high Av, is influenced by various processes including turbulence and selfgravity. The breaks can also be identified, often more readily, in the CMDs. The PDF break from lognormal (Av(SF)» 6–10 mag) appears to shift to higher Av by stellar feedback, so that high-mass star-forming regions tend to have higher PDF breaks. A second break at Av> 50 mag traces structures formed or influenced by a dynamic process. Because such a process has been suggested to drive high-mass star formation in W3, this second break might then identify regions with potential for hosting high-mass stars/clusters. Stellar feedback appears to be a major mechanism driving the local evolution and state of regions within W3. A high initial star formation efficiency in a dense medium could result in a self-enhancing process, leading to more compression and favorable star formation conditions (e.g., colliding flows), a richer stellar content, and massive stars. This scenario would be compatible with the “convergent constructive feedback” model introduced in our previous Herschel study.

Item Type: Journal Item
Copyright Holders: 2015 The American Astronomical Society
ISSN: 1538-4357
Keywords: dust; extinction; infrared; stars; ISM; individual objects (Westerhout 3); stars; early-type; stars; formation
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 45579
Depositing User: G. J. White
Date Deposited: 15 Mar 2016 11:59
Last Modified: 08 Dec 2018 09:59
URI: http://oro.open.ac.uk/id/eprint/45579
Share this page:

Metrics

Altmetrics from Altmetric

Citations from Dimensions

Download history for this item

These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU