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The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X

Roy, Arabindo and Bock, James J. and Noriega-Crespo, Alberto and Viero, Marco P. (2011) The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X. Astrophysical Journal, 727 (2). Art. No. 114. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20110310-135511674

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Abstract

We present Cygnus X in a new multi-wavelength perspective based on an unbiased BLAST survey at 250, 350, and 500 μm, combined with rich data sets for this well-studied region. Our primary goal is to investigate the early stages of high-mass star formation. We have detected 184 compact sources in various stages of evolution across all three BLAST bands. From their well-constrained spectral energy distributions, we obtain the physical properties mass, surface density, bolometric luminosity, and dust temperature. Some of the bright sources reaching 40 K contain well-known compact H_(II) regions. We relate these to other sources at earlier stages of evolution via the energetics as deduced from their position in the luminosity-mass (L-M) diagram. The BLAST spectral coverage, near the peak of the spectral energy distribution of the dust, reveals fainter sources too cool (~10 K) to be seen by earlier shorter-wavelength surveys like IRAS. We detect thermal emission from infrared dark clouds and investigate the phenomenon of cold "starless cores" more generally. Spitzer images of these cold sources often show stellar nurseries, but these potential sites for massive star formation are "starless" in the sense that to date there is no massive protostar in a vigorous accretion phase. We discuss evolution in the context of the L-M diagram. Theory raises some interesting possibilities: some cold massive compact sources might never form a cluster containing massive stars, and clusters with massive stars might not have an identifiable compact cold massive precursor.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/727/2/114DOIUNSPECIFIED
http://iopscience.iop.org/0004-637X/727/2/114/PublisherUNSPECIFIED
Additional Information:© 2011 American Astronomical Society. Received 2010 September 10; accepted 2010 November 18; published 2011 January 11. The BLAST collaboration acknowledges the support of NASA through grant numbers NAG5-12785, NAG5-13301, and NNGO-6GI11G, the Canadian Space Agency (CSA), the UK Particle Physics & Astronomy Research Council (PPARC), and Canada’s Natural Sciences and Engineering Research Council (NSERC). We would also thank the Columbia Scientific Balloon Facility (CSBF) staff for their outstanding work.
Funders:
Funding AgencyGrant Number
NASA NAG5-12785
NASA NAG5-13301
NASA NNGO-6GI11G
Canadian Space Agency (CSA)UNSPECIFIED
Particle Physics and Astronomy Research Council (PPARC) (UK)UNSPECIFIED
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Subject Keywords:balloons; ISM: clouds; stars: formation; stars: massive; submillimeter: general
Issue or Number:2
Classification Code:PACS: 95.80.+p, 97.10.Gz, 95.85.Fm, 97.10.Bt, 98.38.Dq
Record Number:CaltechAUTHORS:20110310-135511674
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20110310-135511674
Official Citation:Arabindo Roy et al. 2011 ApJ 727 114 doi: 10.1088/0004-637X/727/2/114
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:22812
Collection:CaltechAUTHORS
Deposited By: Benjamin Perez
Deposited On:10 Mar 2011 22:24
Last Modified:03 Oct 2019 02:40

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