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Deriving a multivariate α_(CO) conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations

Accurso, G. and Saintonge, A. and Catinella, B. and Cortese, L. and Davé, R. and Dunsheath, S. H. and Genzel, R. and Graciá-Carpio, J. and Heckman, T. M. and Kramer, Jimmy C. and Kramer, C. and Li, Cheng and Lutz, K. and Schiminovich, D. and Schuster, K. and Sternberg, A. and Sturm, E. and Tacconi, L. J. and Tran, K. V. and Wang, J. (2017) Deriving a multivariate α_(CO) conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations. Monthly Notices of the Royal Astronomical Society, 470 (4). pp. 4750-4766. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20170914-084118262

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Abstract

We present Herschel PACS observations of the [C II] 158 μm emission line in a sample of 24 intermediate mass (9 < log M_*/M_⊙ < 10) and low metallicity (0.4 < Z/Z_⊙ < 1.0) galaxies from the xCOLD GASS survey. In combination with IRAM CO (1−0) measurements, we establish scaling relations between integrated and molecular region L_([CII])/L_(CO (1–0)) ratios as a function of integrated galaxy properties. A Bayesian analysis reveals that only two parameters, metallicity and offset from the main sequence, Δ(MS), are needed to quantify variations in the luminosity ratio; metallicity describes the total dust content available to shield CO from UV radiation, while Δ(MS) describes the strength of this radiation field. We connect the L_([CII])/L_(CO (1–0)) ratio to the CO-to-H_2 conversion factor and find a multivariate conversion function, which can be used up to z ∼ 2.5. This function depends primarily on metallicity, with a second-order dependence on Δ(MS). We apply this to the full xCOLD GASS and PHIBSS1 surveys and investigate molecular gas scaling relations. We find a flattening of the relation between gas mass fraction and stellar mass at log M_* < 10.0. While the molecular gas depletion time varies with sSFR, it is mostly independent of mass, indicating that the low L_(CO)/SFR ratios long observed in low-mass galaxies are entirely due to photodissociation of CO and not to an enhanced star formation efficiency.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stx1556DOIArticle
https://arxiv.org/abs/1702.03888arXivDiscussion Paper
https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx1556#supplementary-dataRelated ItemSupplementary Data
ORCID:
AuthorORCID
Cortese, L.0000-0002-7422-9823
Genzel, R.0000-0002-2767-9653
Li, Cheng0000-0002-8280-3119
Tacconi, L. J.0000-0002-1485-9401
Alternate Title:Deriving a multivariate CO-to-H2 conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations
Additional Information:© 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Received: 21 August 2016. Revision Received: 17 June 2017. Accepted: 20 June 2017. Published: 22 June 2017. GA would like to thank the UK Science and Technologies Facilities Council (STFC) for their support via a postgraduate studentship. AS acknowledges the support of the Royal Society through the award of a University Research Fellowship. BC is the recipient of an Australian Research Council Future Fellowship (FT120100660). BC and LC acknowledge support from the Australian Research Councils Discovery Projects funding scheme (DP150101734). This work is based on observations carried out with the IRAM 30m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain). We thank the staff of the telescope for their help in conducting the COLD GASS observations. PACS, aboard Herschel, has been developed by MPE (Germany); UVIE (Austria); KU Leuven, CSL, IMEC (Belgium); CEA, LAM (France); MPIA (Germany); INAF- IFSI/OAA/OAP/OAT, LENS, SISSA (Italy) and IAC (Spain). This development has been supported by BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI/INAF (Italy) and CICYT/MCYT (Spain).
Funders:
Funding AgencyGrant Number
Australian Research Council FT120100660
Australian Research CouncilDP150101734
Institut national des sciences de l'Univers (INSU)UNSPECIFIED
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Max-Planck-Gesellschaft (MPG)UNSPECIFIED
Instituto Geográfico Nacional (IGN)UNSPECIFIED
Bundesministerium für Verkehr, Innovation und Technologie (BMVIT) UNSPECIFIED
ESA-PRODEX (Belgium)UNSPECIFIED
Commissariat à l'énergie atomique (CEA) UNSPECIFIED
Centre National d'Études Spatiales (CNES) UNSPECIFIED
Deutsches Zentrum für Luft- und Raumfahrt (DLR)UNSPECIFIED
Agenzia Spaziale Italiana (ASI) UNSPECIFIED
Istituto Nazionale di Astrofisica (INAF) UNSPECIFIED
Comisión Interministerial de Ciencia y Tecnología (CICYT)UNSPECIFIED
Ministerio de Ciencia Y Tecnologia (MCYT)UNSPECIFIED
Subject Keywords:surveys, galaxies: evolution, galaxies: fundamental parameters, galaxies: ISM, radio lines: galaxies
Issue or Number:4
Record Number:CaltechAUTHORS:20170914-084118262
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170914-084118262
Official Citation:G. Accurso, A. Saintonge, B. Catinella, L. Cortese, R. Davé, S. H. Dunsheath, R. Genzel, J. Gracia-Carpio, T. M. Heckman, Jimmy, C. Kramer, Cheng Li, K. Lutz, D. Schiminovich, K. Schuster, A. Sternberg, E. Sturm, L. J. Tacconi, K. V. Tran, J. Wang; Deriving a multivariate αCO conversion function using the [C II]/CO (1−0) ratio and its application to molecular gas scaling relations, Monthly Notices of the Royal Astronomical Society, Volume 470, Issue 4, 1 October 2017, Pages 4750–4766, https://doi.org/10.1093/mnras/stx1556
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:81436
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:14 Sep 2017 22:10
Last Modified:17 Nov 2019 05:31

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