دورية أكاديمية
Planck intermediate results: XXXI : microwave survey of Galactic supernova remnants
| العنوان: | Planck intermediate results: XXXI : microwave survey of Galactic supernova remnants |
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| المؤلفون: | M. Arnaud, M. Ashdown, F. Atrio Barandela, J. Aumont, C. Baccigalupi, A. J. Banday, R. B. Barreiro, E. Battaner, K. Benabed, A. Benoit Lévy, J. . Bernard, P. Bielewicz, J. Bobin, J. R. Bond, J. Borrill, F. R. Bouchet, C. L. Brogan, C. Burigana, J. . Cardoso, A. Catalano, A. Chamballu, H. C. Chiang, P. R. Christensen, S. Colombi, L. P. L. Colombo, B. P. Crill, A. Curto, F. Cuttaia, R. D. Davies, R. J. Davis, P. De Bernardis, A. De Rosa, G. De Zotti, J. Delabrouille, F. . Désert, C. Dickinson, J. M. Diego, S. Donzelli, O. Doré, X. Dupac, T. A. Enßlin, H. K. Eriksen, F. Finelli, O. Forni, M. Frailis, A. A. Fraisse, E. Franceschi, S. Galeotta, K. Ganga, M. Giard, Y. Giraud Héraud, J. González Nuevo, K. M. Górski, A. Gregorio, A. Gruppuso, F. K. Hansen, D. L. Harrison, C. Hernández Monteagudo, D. Herranz, S. R. Hildebrandt, M. Hobson, W. A. Holmes, K. M. Huffenberger, A. H. Jaffe, T. R. Jaffe, E. Keihänen, R. Keskitalo, T. S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki Suonio, A. Lähteenmäki, J. . Lamarre, A. Lasenby, C. R. Lawrence, R. Leonardi, M. Liguori, P. B. Lilje, M. Linden Vørnle, M. López Caniego, P. M. Lubin, M. Maris, D. J. Marshall, P. G. Martin, E. Martínez González, S. Masi, S. Matarrese, P. Mazzotta, A. Melchiorri, L. Mendes, M. Migliaccio, M. . Miville Deschênes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J. A. Murphy, P. Naselsky, F. Nati, F. Noviello, D. Novikov, I. Novikov, N. Oppermann, C. A. Oxborrow, L. Pagano, F. Pajot, R. Paladini, F. Pasian, M. Peel, O. Perdereau, F. Perrotta, F. Piacentini, M. Piat, D. Pietrobon, S. Plaszczynski, E. Pointecouteau, G. Polenta, L. Popa, G. W. Pratt, J. . Puget, J. P. Rachen, W. T. Reach, W. Reich, M. Reinecke, M. Remazeilles, C. Renault, J. Rho, S. Ricciardi, T. Riller, I. Ristorcelli, G. Rocha, C. Rosset, G. Roudier, B. Rusholme, M. Sandri, G. Savini, D. Scott, V. Stolyarov, D. Sutton, A. . Suur Uski, J. . Sygnet, J. A. Tauber, L. Terenzi, L. Toffolatti, M. Tristram, M. Tucci, G. Umana, L. Valenziano, J. Valiviita, B. Van Tent, P. Vielva, F. Villa, L. A. Wade, D. Yvon, A. Zacchei, A. Zonca, M. Bersanelli, D. Maino, A. Mennella, M. Tomasi |
| المساهمون: | M. Arnaud, M. Ashdown, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, A.J. Banday, R.B. Barreiro, E. Battaner, K. Benabed, A. Benoit-Lévy, J.-. Bernard, M. Bersanelli, P. Bielewicz, J. Bobin, J.R. Bond, J. Borrill, F.R. Bouchet, C.L. Brogan, C. Burigana, J.-. Cardoso, A. Catalano, A. Chamballu, H.C. Chiang, P.R. Christensen, S. Colombi, L.P.L. Colombo, B.P. Crill, A. Curto, F. Cuttaia, R.D. Davie, R.J. Davi, P. De Bernardi, A. De Rosa, G. De Zotti, J. Delabrouille, F.-. Désert, C. Dickinson, J.M. Diego, S. Donzelli, O. Doré, X. Dupac, T.A. Enßlin, H.K. Eriksen, F. Finelli, O. Forni, M. Fraili, A.A. Fraisse, E. Franceschi, S. Galeotta, K. Ganga, M. Giard, Y. Giraud-Héraud, J. González-Nuevo, K.M. Górski, A. Gregorio, A. Gruppuso, F.K. Hansen, D.L. Harrison, C. Hernández-Monteagudo, D. Herranz, S.R. Hildebrandt, M. Hobson, W.A. Holme, K.M. Huffenberger, A.H. Jaffe, T.R. Jaffe, E. Keihänen, R. Keskitalo, T.S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, A. Lähteenmäki, J.-. Lamarre, A. Lasenby, C.R. Lawrence, R. Leonardi, M. Liguori, P.B. Lilje, M. Linden-Vørnle, M. López-Caniego, P.M. Lubin, D. Maino, M. Mari, D.J. Marshall, P.G. Martin, E. Martínez-González, S. Masi, S. Matarrese, P. Mazzotta, A. Melchiorri, L. Mende, A. Mennella, M. Migliaccio, M.-. Miville-Deschêne, A. Moneti, L. Montier, G. Morgante, D. Mortlock |
| بيانات النشر: | EDP Sciences |
| سنة النشر: | 2016 |
| المجموعة: | The University of Milan: Archivio Istituzionale della Ricerca (AIR) |
| مصطلحات موضوعية: | ISM: supernova remnant, cosmic ray, radio continuum: ISM, Settore FIS/05 - Astronomia e Astrofisica |
| الوصف: | The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 16 were detected in at least two Planck frequencies. The radio-through-microwave spectral energy distributions were compiled to determine the mechanism for microwave emission. In only one case, IC 443, is there high-frequency emission clearly from dust associated with the supernova remnant. In all cases, the low-frequency emission is from synchrotron radiation. As predicted for a population of relativistic particles with energy distribution that extends continuously to high energies, a single power law is evident for many sources, including the Crab and PKS 1209-51/52. A decrease in flux density relative to the extrapolation of radio emission is evident in several sources. Their spectral energy distributions can be approximated as broken power laws, Sν ∝ ν-α, with the spectral index, α, increasing by 0.5-1 above a break frequency in the range 10-60 GHz. The break could be due to synchrotron losses. |
| نوع الوثيقة: | article in journal/newspaper |
| اللغة: | English |
| العلاقة: | info:eu-repo/semantics/altIdentifier/wos/WOS:000369715900144; volume:586; firstpage:1; lastpage:21; numberofpages:21; journal:ASTRONOMY & ASTROPHYSICS; http://hdl.handle.net/2434/387621Test; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-84958958774 |
| DOI: | 10.1051/0004-6361/201425022 |
| الإتاحة: | https://doi.org/10.1051/0004-6361/201425022Test http://hdl.handle.net/2434/387621Test |
| حقوق: | info:eu-repo/semantics/openAccess |
| رقم الانضمام: | edsbas.7F3D8A0C |
| قاعدة البيانات: | BASE |
| DOI: | 10.1051/0004-6361/201425022 |
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