The Open UniversitySkip to content
 

The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey. II. Warm molecular gas and star formation in three field spiral galaxies

Warren, B. E.; Wilson, C. D.; Israel, F. P.; Serjeant, S.; Bendo, G. J.; Brinks, E.; Clements, D. L.; Irwin, J. A.; Knapen, J. H.; Leech, J.; Matthews, H. E.; Mühle, S.; Mortimer, A. M. J.; Petitpas, G.; Sinukoff, E.; Spekkens, K.; Tan, B. K.; Tilanus, R. P. J.; Usero, A.; van der Werf, P. P.; Vlahakis, C.; Wiegert, T. and Zhu, M. (2010). The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey. II. Warm molecular gas and star formation in three field spiral galaxies. The Astrophysical Journal, 714(1) pp. 571–588.

Full text available as:
Full text not publicly available
Due to copyright restrictions, this file is not available for public download
Click here to request a copy from the OU Author.
DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1088/0004-637X/714/1/571
Google Scholar: Look up in Google Scholar

Abstract

We present the results of large-area 12CO J = 3-2 emission mapping of three nearby field galaxies, NGC 628, NGC 3521, and NGC 3627, completed at the James Clerk Maxwell Telescope as part of the Nearby Galaxies Legacy Survey. These galaxies all have moderate to strong 12CO J = 3-2 detections over large areas of the fields observed by the survey, showing resolved structure and dynamics in their warm/dense molecular gas disks. All three galaxies were part of the Spitzer Infrared Nearby Galaxies Survey sample, and as such have excellent published multiwavelength ancillary data. These data sets allow us to examine the star formation properties, gas content, and dynamics of these galaxies on sub-kiloparsec scales. We find that the global gas depletion time for dense/warm molecular gas in these galaxies is consistent with other results for nearby spiral galaxies, indicating this may be independent of galaxy properties such as structures, gas compositions, and environments. Similar to the results from The HI Nearby Galaxy Survey, we do not see a correlation of the star formation efficiency with the gas surface density consistent with the Schmidt-Kennicutt law. Finally, we find that the star formation efficiency of the dense molecular gas traced by 12CO J = 3-2 is potentially flat or slightly declining as a function of molecular gas density, the 12CO J = 3-2/J = 1-0 ratio (in contrast to the correlation found in a previous study into the starburst galaxy M83), and the fraction of total gas in molecular form.

Item Type: Journal Article
Copyright Holders: 2010 The American Astronomical Society
ISSN: 1538-4357
Keywords: individual galaxies; NGC 628; NGC 3521; NGC 3627;kinematics and dynamics; spiral galaxies; star formation; molecules
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 25185
Depositing User: Astrid Peterkin
Date Deposited: 15 Dec 2010 10:29
Last Modified: 24 Feb 2014 18:51
URI: http://oro.open.ac.uk/id/eprint/25185
Share this page:

Actions (login may be required)

View Item
Report issue / request change

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340   general-enquiries@open.ac.uk