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-Levy; 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. Desert; C. Dickinson; J. M. Diego; S. Donzelli; O. Dore; 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-Heraud; J. Gonzalez-Nuevo; K. M. Gorski; A. Gregorio; A. Gruppuso; F. K. Hansen; D. L. Harrison; C. Hernandez-Monteagudo; D. Herranz; S. R. Hildebrandt; M. Hobson; W. A. Holmes; K. M. Huffenberger; A. H. Jaffe; T. R. Jaffe; E. Keihaenen; R. Keskitalo; T. S. Kisner; R. Kneissl; J. Knoche; M. Kunz; H. Kurki-Suonio; A. Lahteenmaki; J. -M. Lamarre; A. Lasenby; C. R. Lawrence; R. Leonardi; M. Liguori; P. B. Lilje; M. Linden-Vørnle; M. Lopez-Caniego; P. M. Lubin; D. Maino; 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; M-A Miville-Deschenes; A. Moneti; L. Montier; G. Morgante; D. Mortlock; D. Munshi; J. A. Murphy; P. Naselsky; F. Nati; E. Noviello; D. Novikov; I. Novikov; N. Oppermann; C. A. Oxborrow; L. Pagano; Fernand 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-Levy, 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. Desert, C. Dickinson, J. M. Diego, S. Donzelli, O. Dore, 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-Heraud, J. Gonzalez-Nuevo, K. M. Gorski, A. Gregorio, A. Gruppuso, F. K. Hansen, D. L. Harrison, C. Hernandez-Monteagudo, D. Herranz, S. R. Hildebrandt, M. Hobson, W. A. Holmes, K. M. Huffenberger, A. H. Jaffe, T. R. Jaffe, E. Keihaenen, R. Keskitalo, T. S. Kisner, R. Kneissl, J. Knoche, M. Kunz, H. Kurki-Suonio, A. Lahteenmaki, J. -M. Lamarre, A. Lasenby, C. R. Lawrence, R. Leonardi, M. Liguori, P. B. Lilje, M. Linden-Vørnle, M. Lopez-Caniego, P. M. Lubin, D. Maino, 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, M-A Miville-Deschenes, A. Moneti, L. Montier, G. Morgante, D. Mortlock, D. Munshi, J. A. Murphy, P. Naselsky, F. Nati, E. Noviello, D. Novikov, I. Novikov, N. Oppermann, C. A. Oxborrow, L. Pagano, Fernand 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

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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_v proportional to _v^-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
Article number	A134
Journal	Astronomy and Astrophysics
Volume	586
Number of pages	21
ISSN	0004-6361
DOIs	https://doi.org/10.1051/0004-6361/201425022
Publication status	Published - 2016

Keywords

ISM: supernova remnants
Radio continuum: ISM
Supernova Remnants: Individual: G21.5-0.9, W 44, CTB 80, Cygnus Loop, HB 21, Cas A, Tycho, 3C 58, Crab, IC 443, Puppis A, Vela, PKS 2109-51/52, RCW 86, MSH 15-5 6 , SN 1006

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Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoit-Levy, 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{b877def2031a4028b1462450fbf82b4c,

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, Sv proportional to v-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, Radio continuum: ISM, Supernova Remnants: Individual: G21.5-0.9, W 44, CTB 80, Cygnus Loop, HB 21, Cas A, Tycho, 3C 58, Crab, IC 443, Puppis A, Vela, PKS 2109-51/52, RCW 86, MSH 15-5 6 , SN 1006",

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-Levy 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 Desert, {F. -X.} and C. Dickinson and Diego, {J. M.} and S. Donzelli and O. Dore and X. Dupac and Ensslin, {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-Heraud and J. Gonzalez-Nuevo and Gorski, {K. M.} and A. Gregorio and A. Gruppuso and Hansen, {F. K.} and Harrison, {D. L.} and C. Hernandez-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. Keihaenen and R. Keskitalo and Kisner, {T. S.} and R. Kneissl and J. Knoche and M. Kunz and H. Kurki-Suonio and A. Lahteenmaki 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. Lopez-Caniego and Lubin, {P. M.} and D. Maino and M. Maris and Marshall, {D. J.} and Martin, {P. G.} and E. Martinez-Gonzalez and S. Masi and S. Matarrese and P. Mazzotta and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and M-A Miville-Deschenes 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 E. Noviello and D. Novikov and I. Novikov and N. Oppermann and Oxborrow, {C. A.} and L. Pagano and Fernand 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",

year = "2016",

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

language = "English",

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-Levy, A, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bobin, J, Bond, JR, Borrill, J, Bouchet, FR, Brogan, CL, Burigana, C, Cardoso, J-F, 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, Desert, F-X, Dickinson, C, Diego, JM, Donzelli, S, Dore, O, Dupac, X, Ensslin, TA, Eriksen, HK, Finelli, F, Forni, O, Frailis, M, Fraisse, AA, Franceschi, E, Galeotta, S, Ganga, K, Giard, M, Giraud-Heraud, Y, Gonzalez-Nuevo, J, Gorski, KM, Gregorio, A, Gruppuso, A, Hansen, FK, Harrison, DL, Hernandez-Monteagudo, C, Herranz, D, Hildebrandt, SR, Hobson, M, Holmes, WA, Huffenberger, KM, Jaffe, AH, Jaffe, TR, Keihaenen, E, Keskitalo, R, Kisner, TS, Kneissl, R, Knoche, J, Kunz, M, Kurki-Suonio, H, Lahteenmaki, A, Lamarre, J-M, Lasenby, A, Lawrence, CR, Leonardi, R, Liguori, M, Lilje, PB, Linden-Vørnle, M, Lopez-Caniego, M, Lubin, PM, Maino, D, Maris, M, Marshall, DJ, Martin, PG, Martinez-Gonzalez, E, Masi, S, Matarrese, S, Mazzotta, P, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Miville-Deschenes, M-A, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Munshi, D, Murphy, JA, Naselsky, P, Nati, F, Noviello, E, 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, J-L, 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, A-S, Sygnet, J-F, 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 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-Levy, 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 - Desert, F. -X.

AU - Dickinson, C.

AU - Diego, J. M.

AU - Donzelli, S.

AU - Dore, 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-Heraud, Y.

AU - Gonzalez-Nuevo, J.

AU - Gorski, K. M.

AU - Gregorio, A.

AU - Gruppuso, A.

AU - Hansen, F. K.

AU - Harrison, D. L.

AU - Hernandez-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 - Keihaenen, E.

AU - Keskitalo, R.

AU - Kisner, T. S.

AU - Kneissl, R.

AU - Knoche, J.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lahteenmaki, 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 - Lopez-Caniego, M.

AU - Lubin, P. M.

AU - Maino, D.

AU - Maris, M.

AU - Marshall, D. J.

AU - Martin, P. G.

AU - Martinez-Gonzalez, E.

AU - Masi, S.

AU - Matarrese, S.

AU - Mazzotta, P.

AU - Melchiorri, A.

AU - Mendes, L.

AU - Mennella, A.

AU - Migliaccio, M.

AU - Miville-Deschenes, 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, E.

AU - Novikov, D.

AU - Novikov, I.

AU - Oppermann, N.

AU - Oxborrow, C. A.

AU - Pagano, L.

AU - Pajot, Fernand

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

Y1 - 2016

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, Sv proportional to v-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, Sv proportional to v-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 - Radio continuum: ISM

KW - Supernova Remnants: Individual: G21.5-0.9, W 44, CTB 80, Cygnus Loop, HB 21, Cas A, Tycho, 3C 58, Crab, IC 443, Puppis A, Vela, PKS 2109-51/52, RCW 86, MSH 15-5 6 , SN 1006

U2 - 10.1051/0004-6361/201425022

DO - 10.1051/0004-6361/201425022

M3 - Journal article

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

Keywords

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