Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946
Interstellar dust plays an important role in the formation of molecular gas and the heating and cooling of the interstellar medium. The spatial distribution of the mm-wavelength dust emission from galaxies is largely unexplored. The NIKA2 Guaranteed Time Project IMEGIN (Interpreting the Millimeter E...
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EDP Sciences
2022-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2022/01/epjconf_mmUniverse2021_00016.pdf |
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author | Ejlali G. Adam R. Ade P. Ajeddig H. André P. Artis E. Aussel H. Beelen A. Benoît A. Berta S. Bing L. Bourrion O. Calvo M. Catalano A. de Looze I. De Petris M. Désert F.-X. Doyle S. Driessen E.F. C. Galametz M. Galliano F. Gomez A. Goupy J. Jones A.P. Hughes A. Katsioli S. Kéruzoré F. Kramer C. Ladjelate B. Lagache G. Leclercq S. Lestrade J.-F. Macías-Pérez J.-F. Madden S.C. Maury A. Mauskopf P. Mayet F. Monfardini A. Muñoz-Echeverría M. Nersesian A. Perotto L. Pisano G. Ponthieu N. Revéret V. Rigby A.J. Ritacco A. Romero C. Roussel H. Ruppin F. Schuster K. Shu S. Sievers A. Smith M. W. S. L. Tabatabaei F. S. Tucker C. Xilouris E.M. Zylka R. |
author_facet | Ejlali G. Adam R. Ade P. Ajeddig H. André P. Artis E. Aussel H. Beelen A. Benoît A. Berta S. Bing L. Bourrion O. Calvo M. Catalano A. de Looze I. De Petris M. Désert F.-X. Doyle S. Driessen E.F. C. Galametz M. Galliano F. Gomez A. Goupy J. Jones A.P. Hughes A. Katsioli S. Kéruzoré F. Kramer C. Ladjelate B. Lagache G. Leclercq S. Lestrade J.-F. Macías-Pérez J.-F. Madden S.C. Maury A. Mauskopf P. Mayet F. Monfardini A. Muñoz-Echeverría M. Nersesian A. Perotto L. Pisano G. Ponthieu N. Revéret V. Rigby A.J. Ritacco A. Romero C. Roussel H. Ruppin F. Schuster K. Shu S. Sievers A. Smith M. W. S. L. Tabatabaei F. S. Tucker C. Xilouris E.M. Zylka R. |
author_sort | Ejlali G. |
collection | DOAJ |
description | Interstellar dust plays an important role in the formation of molecular gas and the heating and cooling of the interstellar medium. The spatial distribution of the mm-wavelength dust emission from galaxies is largely unexplored. The NIKA2 Guaranteed Time Project IMEGIN (Interpreting the Millimeter Emission of Galaxies with IRAM and NIKA2) has recently mapped the mm emission in the grand design spiral galaxy NGC6946. By subtracting the contributions from the free-free, synchrotron, and CO line emission, we map the distribution of the pure dust emission at 1:15mm and 2mm. Separating the arm/interarm regions, we find a dominant 2mm emission from interarms indicating the significant role of the general interstellar radiation field in heating the cold dust. Finally, we present maps of the dust mass, temperature, and emissivity index using the Bayesian MCMC modeling of the spectral energy distribution in NGC6946. |
first_indexed | 2024-12-23T11:43:34Z |
format | Article |
id | doaj.art-ee4ca0313764467f97362e1c197c1e31 |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-23T11:43:34Z |
publishDate | 2022-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj.art-ee4ca0313764467f97362e1c197c1e312022-12-21T17:48:24ZengEDP SciencesEPJ Web of Conferences2100-014X2022-01-012570001610.1051/epjconf/202225700016epjconf_mmUniverse2021_00016Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946Ejlali G.0Adam R.1Ade P.2Ajeddig H.3André P.4Artis E.5Aussel H.6Beelen A.7Benoît A.8Berta S.9Bing L.10Bourrion O.11Calvo M.12Catalano A.13de Looze I.14De Petris M.15Désert F.-X.16Doyle S.17Driessen E.F. C.18Galametz M.19Galliano F.20Gomez A.21Goupy J.22Jones A.P.23Hughes A.24Katsioli S.25Kéruzoré F.26Kramer C.27Ladjelate B.28Lagache G.29Leclercq S.30Lestrade J.-F.31Macías-Pérez J.-F.32Madden S.C.33Maury A.34Mauskopf P.35Mayet F.36Monfardini A.37Muñoz-Echeverría M.38Nersesian A.39Perotto L.40Pisano G.41Ponthieu N.42Revéret V.43Rigby A.J.44Ritacco A.45Romero C.46Roussel H.47Ruppin F.48Schuster K.49Shu S.50Sievers A.51Smith M. W. S. L.52Tabatabaei F. S.53Tucker C.54Xilouris E.M.55Zylka R.56School of Astronomy, Institute for Research in Fundamental Sciences (IPM)LLR (Laboratoire Leprince-Ringuet), CNRS, École Polytechnique, Institut Polytechnique de ParisSchool of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéInstitut d’Astrophysique Spatiale (IAS), CNRS, Université Paris SudInstitut Néel, CNRS, Université Grenoble AlpesInstitut de RadioAstronomie Millimétrique (IRAM)Aix Marseille Univ, CNRS, CNES, LAMUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3Institut Néel, CNRS, Université Grenoble AlpesUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3Sterrenkundig Observatorium Universiteit GentDipartimento di Fisica, Sapienza Università di RomaUniv. Grenoble Alpes, CNRS, IPAGSchool of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeInstitut de RadioAstronomie Millimétrique (IRAM)AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéCentro de Astrobiología (CSIC-INTA), Torrejón de ArdozInstitut Néel, CNRS, Université Grenoble AlpesInstitut d’Astrophysique Spatiale (IAS), CNRS, Université Paris SudUniversité de Toulouse, UPS-OMPNational Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote SensingUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3Instituto de Radioastronomía Milimétrica (IRAM)Instituto de Radioastronomía Milimétrica (IRAM)Aix Marseille Univ, CNRS, CNES, LAMInstitut de RadioAstronomie Millimétrique (IRAM)LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Université, UPMCUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéSchool of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3Institut Néel, CNRS, Université Grenoble AlpesUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3National Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote SensingUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3School of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeUniv. Grenoble Alpes, CNRS, IPAGAIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris CitéSchool of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeInstitut d’Astrophysique Spatiale (IAS), CNRS, Université Paris SudDepartment of Physics and Astronomy, University of PennsylvaniaInstitut d’Astrophysique de Paris, Sorbonne Université, CNRS (UMR7095)Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of TechnologyInstitut de RadioAstronomie Millimétrique (IRAM)CaltechInstituto de Radioastronomía Milimétrica (IRAM)School of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeSchool of Astronomy, Institute for Research in Fundamental Sciences (IPM)School of Physics and Astronomy, Cardiff University, Queen’s Buildings, The ParadeNational Observatory of Athens, Institute for Astronomy, Astrophysics, Space Applications and Remote SensingInstitut de RadioAstronomie Millimétrique (IRAM)Interstellar dust plays an important role in the formation of molecular gas and the heating and cooling of the interstellar medium. The spatial distribution of the mm-wavelength dust emission from galaxies is largely unexplored. The NIKA2 Guaranteed Time Project IMEGIN (Interpreting the Millimeter Emission of Galaxies with IRAM and NIKA2) has recently mapped the mm emission in the grand design spiral galaxy NGC6946. By subtracting the contributions from the free-free, synchrotron, and CO line emission, we map the distribution of the pure dust emission at 1:15mm and 2mm. Separating the arm/interarm regions, we find a dominant 2mm emission from interarms indicating the significant role of the general interstellar radiation field in heating the cold dust. Finally, we present maps of the dust mass, temperature, and emissivity index using the Bayesian MCMC modeling of the spectral energy distribution in NGC6946.https://www.epj-conferences.org/articles/epjconf/pdf/2022/01/epjconf_mmUniverse2021_00016.pdf |
spellingShingle | Ejlali G. Adam R. Ade P. Ajeddig H. André P. Artis E. Aussel H. Beelen A. Benoît A. Berta S. Bing L. Bourrion O. Calvo M. Catalano A. de Looze I. De Petris M. Désert F.-X. Doyle S. Driessen E.F. C. Galametz M. Galliano F. Gomez A. Goupy J. Jones A.P. Hughes A. Katsioli S. Kéruzoré F. Kramer C. Ladjelate B. Lagache G. Leclercq S. Lestrade J.-F. Macías-Pérez J.-F. Madden S.C. Maury A. Mauskopf P. Mayet F. Monfardini A. Muñoz-Echeverría M. Nersesian A. Perotto L. Pisano G. Ponthieu N. Revéret V. Rigby A.J. Ritacco A. Romero C. Roussel H. Ruppin F. Schuster K. Shu S. Sievers A. Smith M. W. S. L. Tabatabaei F. S. Tucker C. Xilouris E.M. Zylka R. Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 EPJ Web of Conferences |
title | Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 |
title_full | Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 |
title_fullStr | Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 |
title_full_unstemmed | Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 |
title_short | Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946 |
title_sort | dust emission in galaxies at millimeter wavelengths cooling of star forming regions in ngc6946 |
url | https://www.epj-conferences.org/articles/epjconf/pdf/2022/01/epjconf_mmUniverse2021_00016.pdf |
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