Possible X-ray cocoon emission from GRB 050709

被引：1
作者：
Ogino, Naoki [1 ]
Arimoto, Makoto [1 ,2 ]
Hamidani, Hamid [3 ]
Sakamoto, Takanori [4 ]
Yonetoku, Daisuke [1 ,2 ]
Sawano, Tatsuya [1 ,2 ]
Serino, Motoko [4 ]
Asano, Katsuaki [5 ]
Kawai, Nobuyuki [6 ]
机构：
[1] Kanazawa Univ, Inst Sci & Engn, Fac Math & Phys, Kakuma machi, Kanazawa, Ishikawa 9201192, Japan
[2] Kanazawa Univ, Inst Sci & Engn, Adv Res Ctr Space Sci & Technol, Kakuma-machi, Kanazawa, Ishikawa 9201192, Japan
[3] Tohoku Univ, Grad Sch Sci, Astron Inst, Aramaki Aoba Ku, Sendai, Miyagi 9808578, Japan
[4] Aoyama Gakuin Univ, Coll Sci & Engn, Dept Phys & Math, 5-10-1 Fuchinobe Chuo-ku, Sagamihara, Kanagawa 2525258, Japan
[5] Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwa-no-Ha, Kashiwa, Chiba 2778582, Japan
[6] Tokyo Inst Technol, Grad Sch Sci, 2-12-1 Ookayama Meguro, Tokyo 1528551, Japan
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2024年 / 76卷 / 03期
关键词：
gamma-ray burst: individual (GRB 050709); gravitational waves; stars: neutron; R-PROCESS NUCLEOSYNTHESIS; GRAVITATIONAL-WAVE SOURCE; STAR MERGER GW170817; OFF-AXIS AFTERGLOW; ELECTROMAGNETIC COUNTERPART; EXTENDED EMISSION; OPTICAL AFTERGLOW; REFRESHED SHOCK; VIEWING ANGLE; JET-AFTERGLOW;
D O I：
10.1093/pasj/psae032
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The detection of the short gamma-ray burst (SGRB) 050709 by the HETE-2 satellite opened the door to understanding the nature of SGRBs, offering clues about their emission mechanism and progenitors, with the crucial aid of optical follow-up observations. Here, we revisit the prompt emission of GRB 050709. Our analysis reveals an initial hard spike similar to 200 ms long, followed by a subsequent soft-tail emission lasting similar to 300 ms. These components could be common among other SGRBs originating from binary neutron merger events, such as GW 170817 and GRB 170817A. Detailed temporal and spectral analyses indicate that the soft-tail emission might be attributed to the cocoon formed by the relativistic jet depositing energy into the surrounding material. We find the necessary cocoon parameters at the breakout, as consistent with numerical simulation results. We compared the physical parameters of this cocoon with those of other SGRBs. The relatively higher cocoon pressure and temperature in GRB 050709 may indicate a more on-axis jet compared with GRB 170817A and GRB 150101B.
引用
收藏
页码：550 / 559
页数：10
相关论文
共 107 条
  • [11] A physical background model for the Fermi Gamma-ray Burst Monitor
    Biltzinger, B.
    Kunzweiler, F.
    Greiner, J.
    Toelge, K.
    Burgess, J. Michael
    [J]. ASTRONOMY & ASTROPHYSICS, 2020, 640
  • [12] Short gamma-ray bursts with extended emission from magnetar birth: jet formation and collimation
    Bucciantini, N.
    Metzger, B. D.
    Thompson, T. A.
    Quataert, E.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 419 (02) : 1537 - 1545
  • [13] Fermi GBM Observations of GRB 150101B: A Second Nearby Event with a Short Hard Spike and a Soft Tail
    Burns, E.
    Veres, P.
    Connaughton, V
    Racusin, J.
    Briggs, M. S.
    Christensen, N.
    Goldstein, A.
    Hamburg, R.
    Kocevski, D.
    McEnery, J.
    Bissaldi, E.
    Dal Canton, T.
    Cleveland, W. H.
    Gibby, M. H.
    Hui, C. M.
    von Kienlin, A.
    Mailyan, B.
    Paciesas, W. S.
    Roberts, O. J.
    Siellez, K.
    Stanbro, M.
    Wilson-Hodge, C. A.
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2018, 863 (02)
  • [14] Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source
    Coulter, D. A.
    Foley, R. J.
    Kilpatrick, C. D.
    Drout, M. R.
    Piro, A. L.
    Shappee, B. J.
    Siebert, M. R.
    Simon, J. D.
    Ulloa, N.
    Kasen, D.
    Madore, B. F.
    Murguia-Berthier, A.
    Pan, Y-C.
    Prochaska, J. X.
    Ramirez-Ruiz, E.
    Rest, A.
    Rojas-Bravo, C.
    [J]. SCIENCE, 2017, 358 (6370) : 1556 - 1558
  • [15] Optical emission from GRB 050709: a short/hard GRB in a star-forming galaxy
    Covino, S
    Malesani, D
    Israel, GL
    D'Avanzo, P
    Antonelli, LA
    Chincarini, G
    Fugazza, D
    Conciatore, ML
    Della Valle, M
    Fiore, F
    Guetta, D
    Hurley, K
    Lazzati, D
    Stella, L
    Tagliaferri, G
    Vietri, M
    Campana, S
    Burrows, DN
    D'Elia, V
    Filliatre, P
    Gehrels, N
    Goldoni, P
    Melandri, A
    Mereghetti, S
    Mirabel, IF
    Moretti, A
    Nousek, J
    O'Brien, PT
    Pellizza, LJ
    Perna, R
    Piranomonte, S
    Romano, P
    Zerbi, FM
    [J]. ASTRONOMY & ASTROPHYSICS, 2006, 447 (02): : L5 - L8
  • [16] The evolution of the X-ray afterglow emission of GW 170817/GRB 170817A in XMM-Newton observations
    D'Avanzo, P.
    Campana, S.
    Salafia, O. S.
    Ghirlanda, G.
    Ghisellini, G.
    Melandri, A.
    Bernardini, M. G.
    Branchesi, M.
    Chassande-Mottin, E.
    Covino, S.
    D'Elia, V.
    Nava, L.
    Salvaterra, R.
    Tagliaferri, G.
    Vergani, S. D.
    [J]. ASTRONOMY & ASTROPHYSICS, 2018, 613
  • [17] Observations of the First Electromagnetic Counterpart to a Gravitational-wave Source by the TOROS Collaboration
    Diaz, M. C.
    Macri, L. M.
    Garcia Lambas, D.
    Mendes de Oliveira, C.
    Nilo Castellon, J. L.
    Ribeiro, T.
    Sanchez, B.
    Schoenell, W.
    Abramo, L. R.
    Akras, S.
    Alcaniz, J. S.
    Artola, R.
    Beroiz, M.
    Bonoli, S.
    Cabral, J.
    Camuccio, R.
    Castillo, M.
    Chavushyan, V.
    Coelho, P.
    Colazo, C.
    Costa-Duarte, M. V.
    Cuevas Larenas, H.
    Depoy, D. L.
    Dominguez Romero, M.
    Dultzin, D.
    Fernandez, D.
    Garcia, J.
    Girardini, C.
    Goncalves, D. R.
    Goncalves, T. S.
    Gurovich, S.
    Jimenez-Teja, Y.
    Kanaan, A.
    Lares, M.
    Lopes de Oliveira, R.
    Lopez-Cruz, O.
    Marshall, J. L.
    Melia, R.
    Molino, A.
    Padilla, N.
    Penuela, T.
    Placco, V. M.
    Quinones, C.
    Ramirez Rivera, A.
    Renzi, V.
    Riguccini, L.
    Rios-Lopez, E.
    Rodriguez, H.
    Sampedro, L.
    Schneiter, M.
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2017, 848 (02)
  • [18] A Turnover in the Radio Light Curve of GW170817
    Dobie, Dougal
    Kaplan, David L.
    Murphy, Tara
    Lenc, Emil
    Mooley, Kunal P.
    Lynch, Christene
    Corsi, Alessandra
    Frail, Dale
    Kasliwal, Mansi
    Hallinan, Gregg
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2018, 858 (02)
  • [19] Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis
    Drout, M. R.
    Piro, A. L.
    Shappee, B. J.
    Kilpatrick, C. D.
    Simon, J. D.
    Contreras, C.
    Coulter, D. A.
    Foley, R. J.
    Siebert, M. R.
    Morrell, N.
    Boutsia, K.
    Di Mille, F.
    Holoien, T. W-S.
    Kasen, D.
    Kollmeier, J. A.
    Madore, B. F.
    Monson, A. J.
    Murguia-Berthier, A.
    Pan, Y-C.
    Prochaska, J. X.
    Ramirez-Ruiz, E.
    Rest, A.
    Adams, C.
    Alatalo, K.
    Banados, E.
    Baughman, J.
    Beers, T. C.
    Bernstein, R. A.
    Bitsakis, T.
    Campillay, A.
    Hansen, T. T.
    Higgs, C. R.
    Ji, A. P.
    Maravelias, G.
    Marshall, J. L.
    Bidin, C. Moni
    Prieto, J. L.
    Rasmussen, K. C.
    Rojas-Bravo, C.
    Strom, A. L.
    Ulloa, N.
    Vargas-Gonzalez, J.
    Wan, Z.
    Whitten, D. D.
    [J]. SCIENCE, 2017, 358 (6370) : 1570 - +
  • [20] Short Gamma-Ray Bursts Viewed from Far Off-axis
    Eichler, David
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2018, 869 (01)
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