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. P. 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; 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; 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. M. 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. Maris; 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; F. Perrotta; F. Piacentini; M. Piat; D. Pietrobon; S. Plaszczynski; 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; 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; M. Tucci; G. Umana; L. Valenziano; J. Valiviita; B. Van Tent; P. Vielva; F. Villa; L. A. Wade; D. Yvon; A. Zacchei; A. Zonca

doi:10.1051/0004-6361/201425022

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. P. Bernard, M. Bersanelli, P. Bielewicz, J. Bobin, J. R. Bond, J. Borrill, F. R. Bouchet, C. L. Brogan, C. Burigana, J. F. CardosoA. 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. 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, 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. M. 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. Maris, 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, F. Perrotta, F. Piacentini, M. Piat, D. Pietrobon, S. Plaszczynski, 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, 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, M. Tucci, G. Umana, L. Valenziano, J. Valiviita, B. Van Tent, P. Vielva, F. Villa, L. A. Wade, D. Yvon, A. Zacchei, A. Zonca

Physics

Research output: Contribution to journal › Article › peer-review

26 Scopus citations

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, 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, S_ν ∝ 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.

Original language	English (US)
Article number	A134
Journal	Astronomy and Astrophysics
Volume	586
DOIs	https://doi.org/10.1051/0004-6361/201425022
State	Published - Feb 1 2016

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

ISM: supernova remnants
cosmic rays
radio continuum: ISM

Access to Document

10.1051/0004-6361/201425022

Cite this

Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bobin, J., Bond, J. R., Borrill, J., Bouchet, F. R., Brogan, C. L., Burigana, C., ... Zonca, A. (2016). Planck intermediate results: XXXI. Microwave survey of Galactic supernova remnants. Astronomy and Astrophysics, 586, Article A134. https://doi.org/10.1051/0004-6361/201425022

@article{b18171bc34c54deabadb04b1358458e0,

title = "Planck intermediate results: XXXI. Microwave survey of Galactic supernova remnants",

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, 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.",

keywords = "ISM: supernova remnants, cosmic rays, radio continuum: ISM",

author = "M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and Banday, {A. J.} and Barreiro, {R. B.} and E. Battaner and K. Benabed and A. Benoit-L{\'e}vy and Bernard, {J. P.} and M. Bersanelli and P. Bielewicz and J. Bobin and Bond, {J. R.} and J. Borrill and Bouchet, {F. R.} and Brogan, {C. L.} and C. Burigana and Cardoso, {J. F.} and A. Catalano and A. Chamballu and Chiang, {H. C.} and Christensen, {P. R.} and S. Colombi and Colombo, {L. P.L.} and Crill, {B. P.} and A. Curto and F. Cuttaia and Davies, {R. D.} and Davis, {R. J.} and {De Bernardis}, P. and {De Rosa}, A. and {De Zotti}, G. and J. Delabrouille and D{\'e}sert, {F. X.} and C. Dickinson and Diego, {J. M.} and S. Donzelli and O. Dor{\'e} and X. Dupac and En{\ss}lin, {T. A.} and Eriksen, {H. K.} and F. Finelli and O. Forni and M. Frailis and Fraisse, {A. A.} and E. Franceschi and S. Galeotta and K. Ganga and M. Giard and Y. Giraud-H{\'e}raud and J. Gonz{\'a}lez-Nuevo and G{\'o}rski, {K. M.} and A. Gregorio and A. Gruppuso and Hansen, {F. K.} and Harrison, {D. L.} and C. Hern{\'a}ndez-Monteagudo and D. Herranz and Hildebrandt, {S. R.} and M. Hobson and Holmes, {W. A.} and Huffenberger, {K. M.} and Jaffe, {A. H.} and Jaffe, {T. R.} and E. Keih{\"a}nen and R. Keskitalo and Kisner, {T. S.} and R. Kneissl and J. Knoche and M. Kunz and H. Kurki-Suonio and A. L{\"a}hteenm{\"a}ki and Lamarre, {J. M.} and A. Lasenby and Lawrence, {C. R.} and R. Leonardi and M. Liguori and Lilje, {P. B.} and M. Linden-V{\o}rnle and M. L{\'o}pez-Caniego and Lubin, {P. M.} and D. Maino and M. Maris and Marshall, {D. J.} and Martin, {P. G.} and E. Mart{\'i}nez-Gonz{\'a}lez and S. Masi and S. Matarrese and P. Mazzotta and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and Miville-Desch{\^e}nes, {M. A.} and A. Moneti and L. Montier and G. Morgante and D. Mortlock and D. Munshi and Murphy, {J. A.} and P. Naselsky and F. Nati and F. Noviello and D. Novikov and I. Novikov and N. Oppermann and Oxborrow, {C. A.} and L. Pagano and F. Pajot and R. Paladini and F. Pasian and M. Peel and O. Perdereau and F. Perrotta and F. Piacentini and M. Piat and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and L. Popa and Pratt, {G. W.} and Puget, {J. L.} and Rachen, {J. P.} and Reach, {W. T.} and W. Reich and M. Reinecke and M. Remazeilles and C. Renault and J. Rho and S. Ricciardi and T. Riller and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and B. Rusholme and M. Sandri and G. Savini and D. Scott and V. Stolyarov and D. Sutton and Suur-Uski, {A. S.} and Sygnet, {J. F.} and Tauber, {J. A.} and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and G. Umana and L. Valenziano and J. Valiviita and {Van Tent}, B. and P. Vielva and F. Villa and Wade, {L. A.} and D. Yvon and A. Zacchei and A. Zonca",

note = "Publisher Copyright: {\textcopyright} ESO, 2016.",

year = "2016",

month = feb,

day = "1",

doi = "10.1051/0004-6361/201425022",

language = "English (US)",

volume = "586",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Battaner, E, Benabed, K, Benoit-Lévy, A, Bernard, JP, Bersanelli, M, Bielewicz, P, Bobin, J, Bond, JR, Borrill, J, Bouchet, FR, Brogan, CL, Burigana, C, Cardoso, JF, Catalano, A, Chamballu, A, Chiang, HC, Christensen, PR, Colombi, S, Colombo, LPL, Crill, BP, Curto, A, Cuttaia, F, Davies, RD, Davis, RJ, De Bernardis, P, De Rosa, A, De Zotti, G, Delabrouille, J, Désert, FX, Dickinson, C, Diego, JM, Donzelli, S, Doré, O, Dupac, X, Enßlin, TA, Eriksen, HK, Finelli, F, Forni, O, Frailis, M, Fraisse, AA, Franceschi, E, Galeotta, S, Ganga, K, Giard, M, Giraud-Héraud, Y, González-Nuevo, J, Górski, KM, Gregorio, A, Gruppuso, A, Hansen, FK, Harrison, DL, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, SR, Hobson, M, Holmes, WA, Huffenberger, KM, Jaffe, AH, Jaffe, TR, Keihänen, E, Keskitalo, R, Kisner, TS, Kneissl, R, Knoche, J, Kunz, M, Kurki-Suonio, H, Lähteenmäki, A, Lamarre, JM, Lasenby, A, Lawrence, CR, Leonardi, R, Liguori, M, Lilje, PB, Linden-Vørnle, M, López-Caniego, M, Lubin, PM, Maino, D, Maris, M, Marshall, DJ, Martin, PG, Martínez-González, E, Masi, S, Matarrese, S, Mazzotta, P, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Miville-Deschênes, MA, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Munshi, D, Murphy, JA, Naselsky, P, Nati, F, Noviello, F, Novikov, D, Novikov, I, Oppermann, N, Oxborrow, CA, Pagano, L, Pajot, F, Paladini, R, Pasian, F, Peel, M, Perdereau, O, Perrotta, F, Piacentini, F, Piat, M, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Popa, L, Pratt, GW, Puget, JL, Rachen, JP, Reach, WT, Reich, W, Reinecke, M, Remazeilles, M, Renault, C, Rho, J, Ricciardi, S, Riller, T, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rusholme, B, Sandri, M, Savini, G, Scott, D, Stolyarov, V, Sutton, D, Suur-Uski, AS, Sygnet, JF, Tauber, JA, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Vielva, P, Villa, F, Wade, LA, Yvon, D, Zacchei, A & Zonca, A 2016, 'Planck intermediate results: XXXI. Microwave survey of Galactic supernova remnants', Astronomy and Astrophysics, vol. 586, A134. https://doi.org/10.1051/0004-6361/201425022

TY - JOUR

T1 - Planck intermediate results

T2 - XXXI. Microwave survey of Galactic supernova remnants

AU - Arnaud, M.

AU - Ashdown, M.

AU - Atrio-Barandela, F.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Battaner, E.

AU - Benabed, K.

AU - Benoit-Lévy, A.

AU - Bernard, J. P.

AU - Bersanelli, M.

AU - Bielewicz, P.

AU - Bobin, J.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Brogan, C. L.

AU - Burigana, C.

AU - Cardoso, J. F.

AU - Catalano, A.

AU - Chamballu, A.

AU - Chiang, H. C.

AU - Christensen, P. R.

AU - Colombi, S.

AU - Colombo, L. P.L.

AU - Crill, B. P.

AU - Curto, A.

AU - Cuttaia, F.

AU - Davies, R. D.

AU - Davis, R. J.

AU - De Bernardis, P.

AU - De Rosa, A.

AU - De Zotti, G.

AU - Delabrouille, J.

AU - Désert, F. X.

AU - Dickinson, C.

AU - Diego, J. M.

AU - Donzelli, S.

AU - Doré, O.

AU - Dupac, X.

AU - Enßlin, T. A.

AU - Eriksen, H. K.

AU - Finelli, F.

AU - Forni, O.

AU - Frailis, M.

AU - Fraisse, A. A.

AU - Franceschi, E.

AU - Galeotta, S.

AU - Ganga, K.

AU - Giard, M.

AU - Giraud-Héraud, Y.

AU - González-Nuevo, J.

AU - Górski, K. M.

AU - Gregorio, A.

AU - Gruppuso, A.

AU - Hansen, F. K.

AU - Harrison, D. L.

AU - Hernández-Monteagudo, C.

AU - Herranz, D.

AU - Hildebrandt, S. R.

AU - Hobson, M.

AU - Holmes, W. A.

AU - Huffenberger, K. M.

AU - Jaffe, A. H.

AU - Jaffe, T. R.

AU - Keihänen, E.

AU - Keskitalo, R.

AU - Kisner, T. S.

AU - Kneissl, R.

AU - Knoche, J.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lähteenmäki, A.

AU - Lamarre, J. M.

AU - Lasenby, A.

AU - Lawrence, C. R.

AU - Leonardi, R.

AU - Liguori, M.

AU - Lilje, P. B.

AU - Linden-Vørnle, M.

AU - López-Caniego, M.

AU - Lubin, P. M.

AU - Maino, D.

AU - Maris, M.

AU - Marshall, D. J.

AU - Martin, P. G.

AU - Martínez-González, E.

AU - Masi, S.

AU - Matarrese, S.

AU - Mazzotta, P.

AU - Melchiorri, A.

AU - Mendes, L.

AU - Mennella, A.

AU - Migliaccio, M.

AU - Miville-Deschênes, M. A.

AU - Moneti, A.

AU - Montier, L.

AU - Morgante, G.

AU - Mortlock, D.

AU - Munshi, D.

AU - Murphy, J. A.

AU - Naselsky, P.

AU - Nati, F.

AU - Noviello, F.

AU - Novikov, D.

AU - Novikov, I.

AU - Oppermann, N.

AU - Oxborrow, C. A.

AU - Pagano, L.

AU - Pajot, F.

AU - Paladini, R.

AU - Pasian, F.

AU - Peel, M.

AU - Perdereau, O.

AU - Perrotta, F.

AU - Piacentini, F.

AU - Piat, M.

AU - Pietrobon, D.

AU - Plaszczynski, S.

AU - Pointecouteau, E.

AU - Polenta, G.

AU - Popa, L.

AU - Pratt, G. W.

AU - Puget, J. L.

AU - Rachen, J. P.

AU - Reach, W. T.

AU - Reich, W.

AU - Reinecke, M.

AU - Remazeilles, M.

AU - Renault, C.

AU - Rho, J.

AU - Ricciardi, S.

AU - Riller, T.

AU - Ristorcelli, I.

AU - Rocha, G.

AU - Rosset, C.

AU - Roudier, G.

AU - Rusholme, B.

AU - Sandri, M.

AU - Savini, G.

AU - Scott, D.

AU - Stolyarov, V.

AU - Sutton, D.

AU - Suur-Uski, A. S.

AU - Sygnet, J. F.

AU - Tauber, J. A.

AU - Terenzi, L.

AU - Toffolatti, L.

AU - Tomasi, M.

AU - Tristram, M.

AU - Tucci, M.

AU - Umana, G.

AU - Valenziano, L.

AU - Valiviita, J.

AU - Van Tent, B.

AU - Vielva, P.

AU - Villa, F.

AU - Wade, L. A.

AU - Yvon, D.

AU - Zacchei, A.

AU - Zonca, A.

PY - 2016/2/1

Y1 - 2016/2/1

N2 - 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.

AB - 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.

KW - ISM: supernova remnants

KW - cosmic rays

KW - radio continuum: ISM

UR - http://www.scopus.com/inward/record.url?scp=84958958774&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84958958774&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201425022

DO - 10.1051/0004-6361/201425022

M3 - Article

AN - SCOPUS:84958958774

SN - 0004-6361

VL - 586

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A134

ER -

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

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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