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Non-standard grain properties, dark gas reservoir, and extended submillimeter excess, probed by Herschel in the Large Magellanic Cloud

Galliano, F. and Hony, S. and Bernard, J.-P. and Bot, C. and Madden, S. C. and Roman-Duval, J. and Galametz, M. and Li, A. and Meixner, M. and Engelbracht, C. W. and Lebouteiller, V. and Misselt, K. and Montiel, E. and Panuzzo, P. and Reach, W. T. and Skibba , R. (2011) Non-standard grain properties, dark gas reservoir, and extended submillimeter excess, probed by Herschel in the Large Magellanic Cloud. Astronomy and Astrophysics, 536 . Art. No. A88. ISSN 0004-6361. http://resolver.caltech.edu/CaltechAUTHORS:20120215-075319368

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Abstract

Context. Herschel provides crucial constraints on the IR SEDs of galaxies, allowing unprecedented accuracy on the dust mass estimates. However, these estimates rely on non-linear models and poorly-known optical properties. Aims. In this paper, we perform detailed modelling of the Spitzer and Herschel observations of the LMC, in order to: (i) systematically study the uncertainties and biases affecting dust mass estimates; and to (ii) explore the peculiar ISM properties of the LMC. Methods. To achieve these goals, we have modelled the spatially resolved SEDs with two alternate grain compositions, to study the impact of different submillimetre opacities on the dust mass. We have rigorously propagated the observational errors (noise and calibration) through the entire fitting process, in order to derive consistent parameter uncertainties. Results. First, we show that using the integrated SED leads to underestimating the dust mass by ≃50% compared to the value obtained with sufficient spatial resolution, for the region we studied. This might be the case, in general, for unresolved galaxies. Second, we show that Milky Way type grains produce higher gas-to-dust mass ratios than what seems possible according to the element abundances in the LMC. A spatial analysis shows that this dilemma is the result of an exceptional property: the grains of the LMC have on average a larger intrinsic submm opacity (emissivity index β ≃ 1.7 and opacity κ_(abs)(160 μm) = 1.6 m^2   kg^(-1)) than those of the Galaxy. By studying the spatial distribution of the gas-to-dust mass ratio, we are able to constrain the fraction of unseen gas mass between ≃10, and ≃100% and show that it is not sufficient to explain the gas-to-dust mass ratio obtained with Milky Way type grains. Finally, we confirm the detection of a 500 μm extended emission excess with an average relative amplitude of ≃15%, varying up to 40%. This excess anticorrelates well with the dust mass surface density. Although we do not know the origin of this excess, we show that it is unlikely the result of very cold dust, or CMB fluctuations.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/0004-6361/201117952DOIArticle
http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/abs/2011/12/aa17952-11/aa17952-11.htmlPublisherArticle
ORCID:
AuthorORCID
Galametz, M.0000-0002-0283-8689
Reach, W. T.0000-0001-8362-4094
Additional Information:© 2011 ESO. Received: 25 August 2011. Accepted: 5 October 2011. Published online 16 December 2011. We would like to thank Anthony Jones, Vincent Guillet, Laurent Verstraete, Bruce Draine and Karl Gordon for stimulating discussions on the matter of this paper. We thank the anonymous referee, for his report, and the editor, Malcolm Walmsley, for his careful reading of the paper. We acknowledge extensive use of the Levenberg-Marquardt χ2 minimization routine written by Craig Markwardt. SPIRE has been developed by a consortium of institutes led by Cardiff Univ. (UK) and including Univ. Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, Univ. Sussex (UK); Caltech, JPL, NHSC, Univ. Colorado (USA). This development has been supported by national funding agencies: CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC, UKSA (UK); and NASA (USA).
Funders:
Funding AgencyGrant Number
Canadian Space Agency (CSA)UNSPECIFIED
National Astronomical Observatories, Chinese Academy of Sciences (NAOC) UNSPECIFIED
Commissariat à l’Energie Atomique (CEA)UNSPECIFIED
Centre National d'Études Spatiales (CNES)UNSPECIFIED
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Agenzia Spaziale Italiana (ASI)UNSPECIFIED
Ministerio de Economía y Competitividad (MICINN)UNSPECIFIED
Swedish National Space Board (SNSB)UNSPECIFIED
Science and Technology Facilities Council (STFC)UNSPECIFIED
United Kingdom Space Agency (UKSA)UNSPECIFIED
NASAUNSPECIFIED
Subject Keywords:ISM: abundances; dust, extinction; galaxies: ISM; galaxies: dwarf; Magellanic Clouds; galaxies: starburst
Record Number:CaltechAUTHORS:20120215-075319368
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120215-075319368
Official Citation:Non-standard grain properties, dark gas reservoir, and extended submillimeter excess, probed by Herschel in the Large Magellanic Cloud A88 F. Galliano et al. Published online: 16 December 2011 DOI: http://dx.doi.org/10.1051/0004-6361/201117952
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:29293
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:15 Feb 2012 16:48
Last Modified:17 Aug 2017 04:52

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