Planck early results. XVI. The Planck view of nearby galaxies
Autor: | Lähteenmäki, A., Poutanen, T., Natoli, P., Polenta, G., Bartlett, J.G., Bucher, M., Cardoso, J.-F., Catalano, A., Delabrouille, J., Ganga, K., Giraud-Héraud, Y., Patanchon, G., Piat, M., Rosset, C., Smoot, G.F., Ashdown, M., Hobson, M., Lasenby, A., Stolyarov, V., Bhatia, R., Kneissl, R., Bond, J.R., Miville-Deschênes, M.-A., Banday, A.J., Bernard, J.-P., Forni, O., Giard, M., Montier, L., Pointecouteau, E., Ristorcelli, I., Bock, J.J., Doré, O., Helou, G., Hildebrandt, S.R., Prézeau, G., Rocha, G., Seiffert, M.D., Challinor, A., Shellard, P., Starck, J.-L., Yvon, D., Linden-Vørnle, Michael, Nørgaard-Nielsen, Hans Ulrik, Toffolatti, L., Netterfield, C.B., Scott, D., Juvela, M., Keihänen, E., Keskitalo, R., Kurki-Suonio, H., Jones, W.C., Cayón, L., Knox, L., Leonardi, R., Lubin, P.M., Zonca, A., Wandelt, B.D., Matarrese, S., De Bernardis, P., Masi, S., Melchiorri, A., Piacentini, F., Bersanelli, M., Maino, D., Mennella, A., Tomasi, M., Gregorio, A., Balbi, A., Cabella, P., De Gasperis, G., Mazzotta, P., Vittorio, N., Christensen, P.R., Naselsky, P., Rebolo, R., Rubiño-Martín, J.A., Dupac, X., Mendes, L., Giardino, G., Laureijs, R.J., Tauber, J.A., Partridge, B., Umana, G., Bonaldi, A., De Zotti, G., Frailis, M., Galeotta, S., Maris, M., Pasian, F., Zacchei, A., Burigana, C., Cuttaia, F., De Rosa, A., Finelli, F., Franceschi, E., Gruppuso, A., Mandolesi, N., Morgante, G., Ricciardi, S., Sandri, M., Terenzi, L., Valenziano, L., Villa, F., Donzelli, S., Stivoli, F., Désert, F.-X., Türler, M., Chamballu, A., Clements, D.L., Jaffe, A.H., Mortlock, D., Novikov, D., Rowan-Robinson, M., Chary, R.-R., Rusholme, B., Benoît, A., Aghanim, N., Aumont, J., Dole, H., Douspis, M., Lagache, G., Noviello, F., Pajot, F., Ponthieu, N., Puget, J.-L., Torre, J.-P., Benabed, K., Bouchet, F.R., Colombi, S., Delouis, J.-M., Hivon, E., Moneti, A., Prunet, S., Sygnet, J.-F., Chiang, L.-Y., Efstathiou, G., Gratton, S., Harrison, D., Munshi, D., Hansen, F.K., Hoyland, R.J., Barreiro, R.B., Herranz, D., López-Caniego, M., Martínez-González, E., Vielva, P., Crill, B.P., Górski, K.M., Holmes, W.A., Lawrence, C.R., Wade, L.A., Davies, R.D., Davis, R.J., Dickinson, C., Maffei, B., Peel, M., MacTavish, C.J., Coulais, A., Lamarre, J.-M., Arnaud, M., Madden, S., MacÍas-Pérez, J.F., Perotto, L., Renault, C., Couchot, F., Henrot-Versillé, S., Perdereau, O., Plaszczynski, S., Tristram, M., Borrill, J., Kisner, T.S., Dörl, U., Enßlin, T.A., Hovest, W., Matthai, F., Reinecke, M., Riller, T., Tuovinen, J., Varis, J., Murphy, A., Novikov, I., Savini, G., Baccigalupi, C., Danese, L., González-Nuevo, J., Leach, S., Perrotta, F., Mann, R., Ade, P.A.R., Sudiwala, R., Osborne, S., Reach, W.T., Battaner, E., Huffenberger, K.M. |
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Přispěvatelé: | Universidad de Cantabria, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Hélium : du fondamental aux applications (HELFA), Institut Néel (NEEL), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), PLANCK, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), HELFA - Hélium : du fondamental aux applications, Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Department of Physics, Helsinki Institute of Physics, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Hélium : du fondamental aux applications (NEEL - HELFA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS) |
Jazyk: | angličtina |
Rok vydání: | 2011 |
Předmět: |
Experimental Physics
[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] Astrophysics ism photometry galaxies galaxies: ism infrared galaxies: photometry submillimeter: galaxies infrared: galaxies submillimeter 01 natural sciences galaxies [Infrared] Radiative transfer Astrophysics::Solar and Stellar Astrophysics 010303 astronomy & astrophysics QB Physics Wavelength Galaxies: ISM symbols Cirrus [SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] Infrared Astrophysics - Cosmology and Nongalactic Astrophysics Cosmology and Nongalactic Astrophysics (astro-ph.CO) Galaxies ISM photometry Submillimeter education FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] galaxies [Submillimeter] symbols.namesake Settore FIS/05 - Astronomia e Astrofisica ISM [Galaxies] 0103 physical sciences Emissivity Planck Astrophysics::Galaxy Astrophysics ISM 010308 nuclear & particles physics photometry [Galaxies] Spectral density Astronomy and Astrophysics Galaxies: photometry Infrared: galaxies 115 Astronomy Space science Astrophysics - Astrophysics of Galaxies Redshift Galaxy galaxies: ISM [PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA] Submillimeter: galaxies Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) |
Zdroj: | Astronomy and Astrophysics, 2011, 536, A16 Lähteenmäki, A, Poutanen, T, Natoli, P, Polenta, G, Bartlett, J G, Bucher, M, Cardoso, J-F, Catalano, A, Delabrouille, J, Ganga, K, Giraud-Héraud, Y, Patanchon, G, Piat, M, Rosset, C, Smoot, G F, Ashdown, M, Hobson, M, Lasenby, A, Stolyarov, V, Bhatia, R, Kneissl, R, Bond, J R, Miville-Deschênes, M-A, Banday, A J, Bernard, J-P, Forni, O, Giard, M, Montier, L, Pointecouteau, E, Ristorcelli, I, Bock, J J, Doré, O, Helou, G, Hildebrandt, S R, Prézeau, G, Rocha, G, Seiffert, M D, Challinor, A, Shellard, P, Starck, J-L, Yvon, D, Linden-Vørnle, M, Nørgaard-Nielsen, H U, Toffolatti, L, Netterfield, C B, Scott, D, Juvela, M, Keihänen, E, Keskitalo, R, Kurki-Suonio, H, Poutanen, T, Jones, W C, Cayón, L, Smoot, G F, Knox, L, Leonardi, R, Lubin, P M, Zonca, A, Wandelt, B D, Matarrese, S, De Bernardis, P, Masi, S, Melchiorri, A, Piacentini, F, Bersanelli, M, Maino, D, Mennella, A, Tomasi, M, Gregorio, A, Natoli, P, Balbi, A, Cabella, P, De Gasperis, G, Mazzotta, P, Vittorio, N, Christensen, P R, Naselsky, P, Rebolo, R, Rubiño-Martín, J A, Kneissl, R, Dupac, X, Leonardi, R, Mendes, L, Giardino, G, Laureijs, R J, Leonardi, R, Tauber, J A, Partridge, B, Kurki-Suonio, H, Lähteenmäki, A, Poutanen, T, Umana, G, Bonaldi, A, De Zotti, G, Polenta, G, Frailis, M, Galeotta, S, Maris, M, Mennella, A, Pasian, F, Zacchei, A, Burigana, C, Cuttaia, F, De Rosa, A, Finelli, F, Franceschi, E, Gruppuso, A, Mandolesi, N, Morgante, G, Natoli, P, Ricciardi, S, Sandri, M, Terenzi, L, Valenziano, L, Villa, F, Bersanelli, M, Donzelli, S, Maino, D, Tomasi, M, Stivoli, F, Désert, F-X, Türler, M, Chamballu, A, Clements, D L, Jaffe, A H, Mortlock, D, Novikov, D, Rowan-Robinson, M, Chary, R-R, Ganga, K, Rusholme, B, Benoît, A, Aghanim, N, Aumont, J, Dole, H, Douspis, M, Lagache, G, Miville-Deschênes, M-A, Noviello, F, Pajot, F, Ponthieu, N, Puget, J-L, Torre, J-P, Benabed, K, Bouchet, F R, Cardoso, J-F, Colombi, S, Delouis, J-M, Hivon, E, Moneti, A, Prunet, S, Sygnet, J-F, Wandelt, B D, Chiang, L-Y, Challinor, A, Efstathiou, G, Gratton, S, Harrison, D, Munshi, D, Donzelli, S, Hansen, F K, Hildebrandt, S R, Hoyland, R J, Rebolo, R, Rubiño-Martín, J A, Barreiro, R B, Herranz, D, López-Caniego, M, Martínez-González, E, Vielva, P, Bartlett, J G, Bock, J J, Crill, B P, Doré, O, Górski, K M, Holmes, W A, Keskitalo, R, Lawrence, C R, Prézeau, G, Rocha, G, Seiffert, M D, Wade, L A, Davies, R D, Davis, R J, Dickinson, C, Maffei, B, Peel, M, Ashdown, M, Challinor, A, Gratton, S, Harrison, D, Lasenby, A, MacTavish, C J, Catalano, A, Coulais, A, Lamarre, J-M, Arnaud, M, Madden, S, Starck, J-L, Cardoso, J-F, Hildebrandt, S R, MacÍas-Pérez, J F, Perotto, L, Renault, C, Couchot, F, Henrot-Versillé, S, Perdereau, O, Plaszczynski, S, Tristram, M, Borrill, J, Kisner, T S, Smoot, G F, Banday, A J, Dörl, U, Enßlin, T A, Hovest, W, Matthai, F, Reinecke, M, Riller, T, Tuovinen, J, Varis, J, Murphy, A, Christensen, P R, Naselsky, P, Novikov, I, Crill, B P, Savini, G, Baccigalupi, C, Danese, L, De Zotti, G, González-Nuevo, J, Leach, S, Perrotta, F, Mann, R, Ade, P A R, Munshi, D, Sudiwala, R, Borrill, J, Osborne, S, Banday, A J, Bernard, J-P, Forni, O, Giard, M, Montier, L, Pointecouteau, E, Ristorcelli, I, Reach, W T, Battaner, E, Huffenberger, K M & Górski, K M 2011, ' Planck early results. XVI. The Planck view of nearby galaxies ', Astronomy and Astrophysics, vol. 536, pp. A16 . https://doi.org/10.1051/0004-6361/201116454 Astronomy and Astrophysics-A&A Astronomy and Astrophysics-A&A, EDP Sciences, 2011, 536, pp.A16. ⟨10.1051/0004-6361/201116454⟩ SCOPUS RUO. Repositorio Institucional de la Universidad de Oviedo instname Astronomy and Astrophysics-A&A, 2011, 536, pp.A16. ⟨10.1051/0004-6361/201116454⟩ Digital.CSIC. Repositorio Institucional del CSIC Tuovinen, J, Varis, J, Clements, D L & Planck Collaboration 2011, ' Planck early results. XVI : The Planck view of nearby galaxies ', Astronomy and Astrophysics, vol. 536, A16 . https://doi.org/10.1051/0004-6361/201116454 |
ISSN: | 0004-6361 |
DOI: | 10.1051/0004-6361/201116454 |
Popis: | 16 páginas, 14 figuras, 1 tabla.-- Planck Collaboration: et al. Theall-sky coverage of the Planck Early Release Compact Source Catalogue (ERCSC) provides an unsurpassed survey of galaxies at submillimetre (submm) wavelengths, representing a major improvement in the numbers of galaxies detected, as well as the range of far-IR/submm wavelengths over which they have been observed. We here present the first results on the properties of nearby galaxies using these data. We match the ERCSC catalogue to IRAS-detected galaxies in the Imperial IRAS Faint Source Redshift Catalogue (IIFSCz), so that we can measure the spectral energy distributions (SEDs) of these objects from 60 to 850μm. This produces a list of 1717 galaxies with reliable associations between Planck and IRAS, from which we select a subset of 468 for SED studies, namely those with strong detections in the three highest frequency Planck bands and no evidence of cirrus contamination. The SEDs are fitted using parametric dust models to determine the range of dust temperatures and emissivities. We find evidence for colder dust than has previously been found in external galaxies, with T < 20K. Such cold temperatures are found using both the standard single temperature dust model with variable emissivity β, or a two dust temperature model with β fixed at 2. We also compare our results to studies of distant submm galaxies (SMGs) which have been claimed to contain cooler dust than their local counterparts. We find that including our sample of 468 galaxies significantly reduces the distinction between the two populations. Fits to SEDs of selected objects using more sophisticated templates derived from radiative transfer models confirm the presence of the colder dust found through parametric fitting. We thus conclude that cold (T < 20K) dust is a significant and largely unexplored component of many nearby galaxies. The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and DEISA (EU). |
Databáze: | OpenAIRE |
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