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Planck intermediate results. XIV. Dust emission at millimetre wavelengths in the Galactic plane

  • P. A. R. Ade
  • , N. Aghanim
  • , Marie-Helene Alves
  • , M. Arnaud
  • , M. Ashdown
  • , F. Atrio-Barandela
  • , J. Aumont
  • , C. Baccigalupi
  • , A. J. Banday
  • , R. B. Barreiro
  • , J. G. Bartlett
  • , E. Battaner
  • , K. Benabed
  • , A. Benoit-Levy
  • , J. -P. Bernard
  • , M. Bersanelli
  • , P. Bielewicz
  • , J. Bobin
  • , A. Bonaldi
  • , J. R. Bond
  • J. Borrill, F. R. Bouchet, F. Boulanger, M. Bucher, C. Burigana, R. C. Butler, J. -F. Cardoso, A. Catalano, A. Chamballu, H. C. Chiang, L. -Y. Chiang, P. R. Christensen, D. L. Clements, S. Colombi, L. P. L. Colombo, F. Couchot, B. P. Crill, A. Curto, F. Cuttaia, L. Danese, R. D. Davies, R. J. Davis, P. de Bernardis, A. de Rosa, G. de Zotti, J. Delabrouille, C. Dickinson, J. M. Diego, H. Dole, S. Donzelli, O. Dore, M. Douspis, X. Dupac, T. A. Ensslin, H. K. Eriksen, E. Falgarone, F. Finelli, O. Forni, M. Frailis, E. Franceschi, S. Galeotta, K. Ganga, T. Ghosh, M. Giard, G. Giardino, J. Gonzalez-Nuevo, K. M. Gorski, A. Gregorio, A. Gruppuso, F. K. Hansen, D. Harrison, C. Hernandez-Monteagudo, D. Herranz, S. R. Hildebrandt, E. Hivon, W. A. Holmes, Allan Hornstrup, W. Hovest, A. H. Jaffe, W. C. Jones, M. Juvela, E. Keihanen, R. Keskitalo, T. S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, G. Lagache, A. Lahteenmaki, J. -M. Lamarre, A. Lasenby, R. J. Laureijs, C. R. Lawrence, R. Leonardi, F. Levrier, M. Liguori, P. B. Lilje, Michael Linden-Vørnle, M. Lopez-Caniego, J. F. Macias-Perez, B. Maffei, D. Maino, N. Mandolesi, M. Maris, D. J. Marshall, P. G. Martin, E. Martinez-Gonzalez, S. Masi, S. Matarrese, P. Mazzotta, A. Melchiorri, L. Mendes, A. Mennella, M. Migliaccio, S. Mitra, M. -A. Miville-Deschenes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J. A. Murphy, P. Naselsky, F. Nati, P. Natoli, Hans Ulrik Nørgaard-Nielsen, F. Noviello, D. Novikov, I. Novikov, Carol Anne Oxborrow, L. Pagano, Fernand Pajot, R. Paladini, D. Paoletti, F. Pasian, G. Patanchon, M. Peel, O. Perdereau, F. Perrotta, F. Piacentini, M. Piat, E. Pierpaoli, D. Pietrobon, S. Plaszczynski, E. Pointecouteau, G. Polenta, N. Ponthieu, L. Popa, G. W. Pratt, S. Prunet, J. -L. Puget, J. P. Rachen, W. T. Reach, R. Rebolo, M. Reinecke, M. Remazeilles, C. Renault, S. Ricciardi, T. Riller, I. Ristorcelli, G. Rocha, C. Rosset, J. A. Rubino-Martin, B. Rusholme, M. Sandri, G. Savini, D. Scott, L. D. Spencer, J. -L. Starck, V. Stolyarov, F. Sureau, D. Sutton, A. -S. Suur-Uski, J. -F. Sygnet, J. A. Tauber, D. Tavagnacco, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, L. Valenziano, J. Valiviita, B. Van Tent, L. Verstraete, P. Vielva, F. Villa, N. Vittorio, L. A. Wade, B. D. Wandelt, D. Yvon, A. Zacchei, A. Zonca, Planck Collaboration
    • Cardiff University
    • University of Paris-Sud - University of Paris XI
    • Université Paris Cité
    • Kavli Institute for Cosmology Cambridge
    • University of Salamanca
    • International School for Advanced Studies
    • Université Fédérale Toulouse Midi-Pyrénées
    • Universidad de Cantabria
    • California Institute of Technology
    • University of Granada
    • Pierre and Marie Curie University - University of Paris VI
    • National Institute for Astrophysics
    • University of Manchester
    • University of Toronto
    • University of California at Berkeley
    • École des mines Paris
    • University Joseph Fourier
    • Princeton University
    • Academia Sinica Taiwan HQ
    • Niels Bohr Institute
    • Imperial College London
    • University of Rome La Sapienza
    • European Space Astronomy Centre
    • Max Planck Institute
    • University of Oslo
    • Observatoire de Paris
    • National Institute for Nuclear Physics
    • European Space Agency - ESA
    • Lawrence Berkeley National Laboratory
    • University of Padua
    • University of Rome Tor Vergata
    • Université Paris-Sud
    • National University of Ireland
    • University of Southern California
    • Institute for Space Sciences
    • Universities Space Research Association
    • Instituto de Astrofísica de Canarias
    • University College London
    • Russian Academy of Sciences
    • CNRS
    • French Alternative Energies and Atomic Energy Commission
    • University of California at Santa Barbara
    • European Southern Observatory
    • University of Helsinki
    • University of British Columbia

    Research output: Contribution to journal › Journal article › Research › peer-review

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    Abstract

    We use Planck HFI data combined with ancillary radio data to study the emissivity index of the interstellar dust emission in the frequency range 100-353 GHz, or 3-0.8 mm, in the Galactic plane. We analyse the region l = 20 degrees-44 degrees and vertical bar b vertical bar
    Original languageEnglish
    Article numberA45
    JournalAstronomy and Astrophysics
    Volume564
    Number of pages13
    ISSN0004-6361
    DOIs
    Publication statusPublished - 2014

    Keywords

    • ASTRONOMY
    • PRE-LAUNCH STATUS
    • SPECTRAL ENERGY-DISTRIBUTIONS
    • MU-M
    • MAGNETIC NANOPARTICLES
    • TEMPERATURE-DEPENDENCE
    • MICROWAVE EMISSION
    • INTERSTELLAR DUST
    • MAGELLANIC-CLOUD
    • MOLECULAR CLOUDS
    • GAL OBSERVATIONS
    • ISM: general
    • Galaxy: general
    • radiation mechanisms: general
    • radio continuum: ISM
    • submillimeter: ISM
    • astro-ph.GA astro-ph.CO

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