Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants - IN2P3 - Institut national de physique nucléaire et de physique des particules
Journal Articles Astronomy & Astrophysics - A&A Year : 2016

Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants

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. -F. Cardoso , A. Catalano (1) , 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. -X. Désert , C. Dickinson , J. M. Diego , S. Donzelli , O. Doré , X. Dupac , T. A. Ensslin , H. K. Eriksen , F. Finelli , O. Forni , M. Frailis , E. Franceschi , S. Galeotta , K. Ganga , M. Giard , Y. Giraud-Héraud , J. González-Nuevo , K. M. Górski , D. A. Green , A. Gregorio , A. Gruppuso , F. K. Hansen , D. L. Harrison , C. Hernández-Monteagudo , D. Herranz , S. R. Hildebrandt , 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. -M. Lamarre , A. Lasenby , C. R. Lawrence , R. Leonardi , M. Liguori , P. B. Lilje , M. Linden-Vørnle , P. M. Lubin , D. Maino , D. J. Marshall , P. G. Martin , E. Martínez-González , S. Masi , S. Matarrese , P. Mazzotta , A. Melchiorri , L. Mendes , A. Mennella , M. Migliaccio , M. -A. 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 (2) , F. Perrotta , F. Piacentini , M. Piat , D. Pietrobon , Stéphane Plaszczynski (2) , E. Pointecouteau , G. Polenta , L. Popa , G. W. Pratt , J. -L. Puget , J. P. Rachen , W. T. Reach , W. Reich , M. Reinecke , M. Remazeilles , C. Renault (1) , 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. -S. Suur-Uski , J. -F. Sygnet , J. A. Tauber , L. Terenzi , L. Toffolatti , M. Tomasi , M. Tristram (2) , M. Tucci (2) , G. Umana , L. Valenziano , B. van Tent , P. Vielva , Francesca Villa , L. A. Wade , D. Yvon , A. Zacchei , A. Zonca
M. Arnaud
  • Function : Author
M. Ashdown
  • Function : Author
F. Atrio-Barandela
  • Function : Author
J. Aumont
C. Baccigalupi
  • Function : Author
A. J. Banday
R. B. Barreiro
  • Function : Author
E. Battaner
  • Function : Author
K. Benabed
  • Function : Author
A. Benoit-Lévy
  • Function : Author
J. Bernard
  • Function : Author
M. Bersanelli
  • Function : Author
P. Bielewicz
  • Function : Author
J. Bobin
  • Function : Author
J. R. Bond
  • Function : Author
J. Borrill
  • Function : Author
F. R. Bouchet
C. L. Brogan
  • Function : Author
C. Burigana
  • Function : Author
J. -F. Cardoso
A. Chamballu
  • Function : Author
H. C. Chiang
  • Function : Author
P. R. Christensen
  • Function : Author
S. Colombi
  • Function : Author
L. P. L. Colombo
  • Function : Author
B. P. Crill
  • Function : Author
A. Curto
  • Function : Author
F. Cuttaia
  • Function : Author
R. D. Davies
  • Function : Author
R. J. Davis
  • Function : Author
P. de Bernardis
  • Function : Author
A. de Rosa
  • Function : Author
G. de Zotti
  • Function : Author
J. Delabrouille
  • Function : Author
F. -X. Désert
  • Function : Author
C. Dickinson
  • Function : Author
J. M. Diego
  • Function : Author
S. Donzelli
  • Function : Author
O. Doré
  • Function : Author
X. Dupac
  • Function : Author
T. A. Ensslin
  • Function : Author
H. K. Eriksen
  • Function : Author
F. Finelli
O. Forni
M. Frailis
  • Function : Author
E. Franceschi
  • Function : Author
S. Galeotta
  • Function : Author
K. Ganga
  • Function : Author
M. Giard
  • Function : Author
Y. Giraud-Héraud
  • Function : Author
J. González-Nuevo
  • Function : Author
K. M. Górski
  • Function : Author
D. A. Green
  • Function : Author
A. Gregorio
  • Function : Author
A. Gruppuso
  • Function : Author
F. K. Hansen
  • Function : Author
D. L. Harrison
  • Function : Author
C. Hernández-Monteagudo
  • Function : Author
D. Herranz
  • Function : Author
S. R. Hildebrandt
  • Function : Author
W. A. Holmes
  • Function : Author
K. M. Huffenberger
  • Function : Author
A. H. Jaffe
  • Function : Author
T. R. Jaffe
  • Function : Author
E. Keihänen
  • Function : Author
R. Keskitalo
  • Function : Author
T. S. Kisner
  • Function : Author
R. Kneissl
  • Function : Author
J. Knoche
  • Function : Author
M. Kunz
  • Function : Author
H. Kurki-Suonio
  • Function : Author
A. Lähteenmäki
J. -M. Lamarre
  • Function : Author
A. Lasenby
  • Function : Author
C. R. Lawrence
  • Function : Author
R. Leonardi
  • Function : Author
M. Liguori
  • Function : Author
P. B. Lilje
  • Function : Author
M. Linden-Vørnle
  • Function : Author
P. M. Lubin
  • Function : Author
D. Maino
  • Function : Author
D. J. Marshall
  • Function : Author
P. G. Martin
  • Function : Author
E. Martínez-González
  • Function : Author
S. Masi
  • Function : Author
S. Matarrese
  • Function : Author
P. Mazzotta
  • Function : Author
A. Melchiorri
  • Function : Author
L. Mendes
  • Function : Author
A. Mennella
  • Function : Author
M. Migliaccio
  • Function : Author
M. -A. Miville-Deschênes
A. Moneti
  • Function : Author
L. Montier
  • Function : Author
G. Morgante
  • Function : Author
D. Mortlock
  • Function : Author
D. Munshi
  • Function : Author
J. A. Murphy
  • Function : Author
P. Naselsky
  • Function : Author
F. Nati
F. Noviello
  • Function : Author
D. Novikov
  • Function : Author
I. Novikov
  • Function : Author
N. Oppermann
  • Function : Author
C. A. Oxborrow
  • Function : Author
L. Pagano
  • Function : Author
F. Pajot
R. Paladini
F. Pasian
  • Function : Author
M. Peel
  • Function : Author
F. Perrotta
  • Function : Author
F. Piacentini
  • Function : Author
M. Piat
  • Function : Author
D. Pietrobon
  • Function : Author
E. Pointecouteau
G. Polenta
  • Function : Author
L. Popa
  • Function : Author
G. W. Pratt
  • Function : Author
J. -L. Puget
  • Function : Author
J. P. Rachen
  • Function : Author
W. T. Reach
  • Function : Author
W. Reich
  • Function : Author
M. Reinecke
  • Function : Author
M. Remazeilles
  • Function : Author
J. Rho
  • Function : Author
S. Ricciardi
  • Function : Author
T. Riller
  • Function : Author
I. Ristorcelli
  • Function : Author
G. Rocha
  • Function : Author
C. Rosset
  • Function : Author
G. Roudier
  • Function : Author
B. Rusholme
  • Function : Author
M. Sandri
  • Function : Author
G. Savini
  • Function : Author
D. Scott
  • Function : Author
V. Stolyarov
D. Sutton
  • Function : Author
A. -S. Suur-Uski
  • Function : Author
J. -F. Sygnet
  • Function : Author
J. A. Tauber
  • Function : Author
L. Terenzi
  • Function : Author
L. Toffolatti
  • Function : Author
M. Tomasi
  • Function : Author
G. Umana
  • Function : Author
L. Valenziano
  • Function : Author
B. van Tent
  • Function : Author
P. Vielva
  • Function : Author
Francesca Villa
  • Function : Author
L. A. Wade
  • Function : Author
D. Yvon
  • Function : Author
A. Zacchei
  • Function : Author
A. Zonca
  • Function : Author

Abstract

The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 17 were detected in at least two Planck frequencies. The radio-through-microwave spectral energy distributions were compiled to determine the emission mechanism for microwave emission. In only one case, IC 443, is the high-frequency emission clearly from dust associated with the supernova remnant. In all cases, the low-frequency emission is from synchrotron radiation. A single power law, as predicted for a population of relativistic particles with energy distribution that extends continuously to high energies, 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, $S_\nu\propto\nu^{-\alpha}$, with the spectral index, $\alpha$, with the spectral index, alpha, increasing by 0.5 to 1 above a break frequency in the range 10 to 60 GHz. The break could be due to synchrotron losses.

Dates and versions

in2p3-01217094 , version 1 (19-10-2015)

Identifiers

Cite

M. Arnaud, M. Ashdown, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, et al.. Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants. Astronomy & Astrophysics - A&A, 2016, 586, pp.A134. ⟨10.1051/0004-6361/201425022⟩. ⟨in2p3-01217094⟩
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