Burton, Michael G., Ashley, Michael C. B., Braiding, Catherine ORCID: 0000-0002-6475-0797, Storey, John W. V., Kulesa, Craig, Hollenbach, David J., Wolfire, Mark, Glueck, Christian and Rowell, Gavin ORCID: 0000-0002-9516-1581 (2014). THE CARBON INVENTORY IN A QUIESCENT, FILAMENTARY MOLECULAR CLOUD IN G328. Astrophys. J., 782 (2). BRISTOL: IOP PUBLISHING LTD. ISSN 1538-4357

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Abstract

We present spectral line images of [CI] 809 GHz, CO J = 1-0 115 GHz and Hi 1.4 GHz line emission, and calculate the corresponding C, CO and H column densities, for a sinuous, quiescent giant molecular cloud about 5 kpc distant along the l = 328 degrees sightline (hereafter G328) in our Galaxy. The [CI] data comes from the High Elevation Antarctic Terahertz telescope, a new facility on the summit of the Antarctic plateau where the precipitable water vapor falls to the lowest values found on the surface of the Earth. The CO and Hi data sets come from the Mopra and Parkes/ATCA telescopes, respectively. We identify a filamentary molecular cloud, similar to 75 x 5 pc long with mass similar to 4 x 10(4) M-circle dot and a narrow velocity emission range of just 4 km s(-1). The morphology and kinematics of this filament are similar in CO, [CI], and Hi, though in the latter appears as self-absorption. We calculate line fluxes and column densities for the three emitting species, which are broadly consistent with a photodissociation region model for a GMC exposed to the average interstellar radiation field. The [C/CO] abundance ratio averaged through the filament is found to be approximately unity. The G328 filament is constrained to be cold (T-Dust < 20 K) by the lack of far-IR emission, to show no clear signs of star formation, and to only be mildly turbulent from the narrow line width. We suggest that it may represent a GMC shortly after formation, or perhaps still in the process of formation.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Burton, Michael G.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Ashley, Michael C. B.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Braiding, CatherineUNSPECIFIEDorcid.org/0000-0002-6475-0797UNSPECIFIED
Storey, John W. V.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Kulesa, CraigUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Hollenbach, David J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Wolfire, MarkUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Glueck, ChristianUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Rowell, GavinUNSPECIFIEDorcid.org/0000-0002-9516-1581UNSPECIFIED
URN: urn:nbn:de:hbz:38-445757
DOI: 10.1088/0004-637X/782/2/72
Journal or Publication Title: Astrophys. J.
Volume: 782
Number: 2
Date: 2014
Publisher: IOP PUBLISHING LTD
Place of Publication: BRISTOL
ISSN: 1538-4357
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
COSMIC-RAY IONIZATION; DIFFUSE INTERSTELLAR-MEDIUM; FAR-INFRARED LUMINOSITY; GALACTIC PLANE SURVEY; COLOGNE DATABASE; STAR-FORMATION; LINE EMISSION; MILKY-WAY; C-II; REGIONSMultiple languages
Astronomy & AstrophysicsMultiple languages
URI: http://kups.ub.uni-koeln.de/id/eprint/44575

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