Energetic young pulsars and expanding blast waves [ supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma- Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma- ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 x 10(-13) seconds per second. Its characteristic age of 10(4) years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma- ray sources associated with star- forming regions and SNRs are such young pulsars.

The Fermi Gamma-Ray Space Telescope Discovers the Pulsar in the Young Galactic Supernova Remnant CTA 1 / Abdo, Aa; Ackermann, M; Atwood, Wb; Baldini, L; Ballet, J; Barbiellini, G; Baring, Mg; Bastieri, D; Baughman, Bm; Bechtol, K; Bellazzini, R; Berenji, B; Blandford, Rd; Bloom, Ed; Bogaert, G; Bonamente, E; Borgland, Aw; Bregeon, J; Brez, A; Brigida, M; Bruel, P; Burnett, Th; Caliandro, Ga; Cameron, Ra; Caraveo, Pa; Carlson, P; Casandjian, Jm; Cecchi, C; Charles, E; Chekhtman, A; Cheung, Cc; Chiang, J; Ciprini, S; Claus, R; Cohen Tanugi, J; Cominsky, Lr; Conrad, J; Cutini, S; Davis, Ds; Dermer, Cd; de Angelis, A; de Palma, F; Digel, Sw; Dormody, M; Silva, Ede; Drell, Ps; Dubois, R; Dumora, D; Edmonds, Y; Farnier, C; Focke, Wb; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gasparrini, D; Gehrels, N; Germani, S; Giebels, B; Giglietto, Nicola; Giordano, F; Glanzman, T; Godfrey, G; Grenier, Ia; Grondin, Mh; Grove, Je; Guillemot, L; Guiriec, S; Harding, Ak; Hartman, Rc; Hays, E; Hughes, Re; Johannesson, G; Johnson, As; Johnson, Rp; Johnson, Tj; Johnson, Wn; Kamae, T; Kanai, Y; Kanbach, G; Katagiri, H; Kawai, N; Kerr, M; Kishishita, T; Kiziltan, B; Knodlseder, J; Kocian, Ml; Komin, N; Kuehn, F; Kuss, M; Latronico, L; Lemoine Goumard, M; Longo, F; Lonjou, V; Loparco, F; Lott, B; Lovellette, Mn; Lubrano, P; Makeev, A; Marelli, M; Mazziotta, Mn; Mcenery, Je; Mcglynn, S; Meurer, C; Michelson, Pf; Mineo, T; Mitthumsiri, W; Mizuno, T; Moiseev, Aa; Monte, C; Monzani, Me; Morselli, A; Moskalenko, Iv; Murgia, S; Nakamori, T; Nolan, Pl; Nuss, E; Ohno, M; Ohsugi, T; Okumura, A; Omodei, N; Orlando, E; Ormes, Jf; Ozaki, M; Paneque, D; Panetta, Jh; Parent, D; Pelassa, V; Pepe, M; Pesce Rollins, M; Piano, G; Pieri, L; Piron, F; Porter, Ta; Raino, S; Rando, R; Ray, Ps; Razzano, M; Reimer, A; Reimer, O; Reposeur, T; Ritz, S; Rochester, Ls; Rodriguez, Ay; Romani, Rw; Roth, M; Ryde, F; Sadrozinski, Hfw; Sanchez, D; Sander, A; Parkinson, Pms; Schalk, Tl; Sellerholm, A; Sgro, C; Siskind, Ej; Smith, Da; Smith, Pd; Spandre, G; Spinelli, P; Starck, Jl; Strickman, Ms; Suson, Dj; Tajima, H; Takahashi, H; Takahashi, T; Tanaka, T; Thayer, Jb; Thayer, Jg; Thompson, Dj; Thorsett, Se; Tibaldo, L; Torres, Df; Tosti, G; Tramacere, A; Usher, Tl; Van Etten, A; Vilchez, N; Vitale, V; Wang, P; Watters, K; Winer, Bl; Wood, Ks; Yasuda, H; Ylinen, T; Ziegler, M.. - In: SCIENCE. - ISSN 0036-8075. - STAMPA. - 322:5905(2008), pp. 1218-1221. [10.1126/science.1165572]

The Fermi Gamma-Ray Space Telescope Discovers the Pulsar in the Young Galactic Supernova Remnant CTA 1

GIGLIETTO, Nicola;
2008-01-01

Abstract

Energetic young pulsars and expanding blast waves [ supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma- Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma- ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 x 10(-13) seconds per second. Its characteristic age of 10(4) years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma- ray sources associated with star- forming regions and SNRs are such young pulsars.
2008
The Fermi Gamma-Ray Space Telescope Discovers the Pulsar in the Young Galactic Supernova Remnant CTA 1 / Abdo, Aa; Ackermann, M; Atwood, Wb; Baldini, L; Ballet, J; Barbiellini, G; Baring, Mg; Bastieri, D; Baughman, Bm; Bechtol, K; Bellazzini, R; Berenji, B; Blandford, Rd; Bloom, Ed; Bogaert, G; Bonamente, E; Borgland, Aw; Bregeon, J; Brez, A; Brigida, M; Bruel, P; Burnett, Th; Caliandro, Ga; Cameron, Ra; Caraveo, Pa; Carlson, P; Casandjian, Jm; Cecchi, C; Charles, E; Chekhtman, A; Cheung, Cc; Chiang, J; Ciprini, S; Claus, R; Cohen Tanugi, J; Cominsky, Lr; Conrad, J; Cutini, S; Davis, Ds; Dermer, Cd; de Angelis, A; de Palma, F; Digel, Sw; Dormody, M; Silva, Ede; Drell, Ps; Dubois, R; Dumora, D; Edmonds, Y; Farnier, C; Focke, Wb; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gasparrini, D; Gehrels, N; Germani, S; Giebels, B; Giglietto, Nicola; Giordano, F; Glanzman, T; Godfrey, G; Grenier, Ia; Grondin, Mh; Grove, Je; Guillemot, L; Guiriec, S; Harding, Ak; Hartman, Rc; Hays, E; Hughes, Re; Johannesson, G; Johnson, As; Johnson, Rp; Johnson, Tj; Johnson, Wn; Kamae, T; Kanai, Y; Kanbach, G; Katagiri, H; Kawai, N; Kerr, M; Kishishita, T; Kiziltan, B; Knodlseder, J; Kocian, Ml; Komin, N; Kuehn, F; Kuss, M; Latronico, L; Lemoine Goumard, M; Longo, F; Lonjou, V; Loparco, F; Lott, B; Lovellette, Mn; Lubrano, P; Makeev, A; Marelli, M; Mazziotta, Mn; Mcenery, Je; Mcglynn, S; Meurer, C; Michelson, Pf; Mineo, T; Mitthumsiri, W; Mizuno, T; Moiseev, Aa; Monte, C; Monzani, Me; Morselli, A; Moskalenko, Iv; Murgia, S; Nakamori, T; Nolan, Pl; Nuss, E; Ohno, M; Ohsugi, T; Okumura, A; Omodei, N; Orlando, E; Ormes, Jf; Ozaki, M; Paneque, D; Panetta, Jh; Parent, D; Pelassa, V; Pepe, M; Pesce Rollins, M; Piano, G; Pieri, L; Piron, F; Porter, Ta; Raino, S; Rando, R; Ray, Ps; Razzano, M; Reimer, A; Reimer, O; Reposeur, T; Ritz, S; Rochester, Ls; Rodriguez, Ay; Romani, Rw; Roth, M; Ryde, F; Sadrozinski, Hfw; Sanchez, D; Sander, A; Parkinson, Pms; Schalk, Tl; Sellerholm, A; Sgro, C; Siskind, Ej; Smith, Da; Smith, Pd; Spandre, G; Spinelli, P; Starck, Jl; Strickman, Ms; Suson, Dj; Tajima, H; Takahashi, H; Takahashi, T; Tanaka, T; Thayer, Jb; Thayer, Jg; Thompson, Dj; Thorsett, Se; Tibaldo, L; Torres, Df; Tosti, G; Tramacere, A; Usher, Tl; Van Etten, A; Vilchez, N; Vitale, V; Wang, P; Watters, K; Winer, Bl; Wood, Ks; Yasuda, H; Ylinen, T; Ziegler, M.. - In: SCIENCE. - ISSN 0036-8075. - STAMPA. - 322:5905(2008), pp. 1218-1221. [10.1126/science.1165572]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/324
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