Are short GRBs really hard?

T. Sakamoto, L. Barbier, S. Barthelmy, J. Cummings, E. Fenimore, N. Gehrels, D. Hullinger, H. Krimm, C. Markwardt, D. Palmer, A. Parsons, G. Sato, J. Tueller, R. Aptekar, T. Cline, S. Golenetskii, E. Mazets, V. Pal'Shin, G. Ricker, D. LambJ. L. Atteia, N. Kawai

Research output: Chapter in Book/Report/Conference proceedingConference contribution

3 Citations (Scopus)

Abstract

Thanks to the rapid position notice and response by HETE-2 and Swift, the X-ray afterglow emissions have been found for four recent short gamma-ray bursts (GRBs; GRB 050509b, GRB 050709, GRB 050724, and GRB 050813). The positions of three out of four short GRBs are coincident with galaxies with no current or recent star formation. This discovery tightens the case for a different origin for short and long GRBs. On the other hand, from the prompt emission point of view, a short GRB shows a harder spectrum comparing to that of the long duration GRBs according to the BATSE observations. We investigate the prompt emission properties of four short GRBs observed by Swift/BAT. We found that the hardness of all four BAT short GRBs is in between the BATSE range for short and long GRBs. We will discuss the spectral properties of short GRBs including the short GRB sample of Konus-Wind and HETE-2 to understand the hard nature of the BATSE short GRBs.

Original languageEnglish
Title of host publicationAIP Conference Proceedings
Pages43-47
Number of pages5
Volume836
DOIs
Publication statusPublished - 2006 May 19
EventGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C.
Duration: 2005 Nov 292005 Dec 2

Other

OtherGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference
CityWashington, D.C.
Period05/11/2905/12/2

Fingerprint

afterglows
gamma ray bursts
star formation
hardness
galaxies
x rays

Keywords

  • Prompt gamma-ray emission
  • Short GRBs

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Sakamoto, T., Barbier, L., Barthelmy, S., Cummings, J., Fenimore, E., Gehrels, N., ... Kawai, N. (2006). Are short GRBs really hard? In AIP Conference Proceedings (Vol. 836, pp. 43-47) https://doi.org/10.1063/1.2207855

Are short GRBs really hard? / Sakamoto, T.; Barbier, L.; Barthelmy, S.; Cummings, J.; Fenimore, E.; Gehrels, N.; Hullinger, D.; Krimm, H.; Markwardt, C.; Palmer, D.; Parsons, A.; Sato, G.; Tueller, J.; Aptekar, R.; Cline, T.; Golenetskii, S.; Mazets, E.; Pal'Shin, V.; Ricker, G.; Lamb, D.; Atteia, J. L.; Kawai, N.

AIP Conference Proceedings. Vol. 836 2006. p. 43-47.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Sakamoto, T, Barbier, L, Barthelmy, S, Cummings, J, Fenimore, E, Gehrels, N, Hullinger, D, Krimm, H, Markwardt, C, Palmer, D, Parsons, A, Sato, G, Tueller, J, Aptekar, R, Cline, T, Golenetskii, S, Mazets, E, Pal'Shin, V, Ricker, G, Lamb, D, Atteia, JL & Kawai, N 2006, Are short GRBs really hard? in AIP Conference Proceedings. vol. 836, pp. 43-47, GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference, Washington, D.C., 05/11/29. https://doi.org/10.1063/1.2207855
Sakamoto T, Barbier L, Barthelmy S, Cummings J, Fenimore E, Gehrels N et al. Are short GRBs really hard? In AIP Conference Proceedings. Vol. 836. 2006. p. 43-47 https://doi.org/10.1063/1.2207855
Sakamoto, T. ; Barbier, L. ; Barthelmy, S. ; Cummings, J. ; Fenimore, E. ; Gehrels, N. ; Hullinger, D. ; Krimm, H. ; Markwardt, C. ; Palmer, D. ; Parsons, A. ; Sato, G. ; Tueller, J. ; Aptekar, R. ; Cline, T. ; Golenetskii, S. ; Mazets, E. ; Pal'Shin, V. ; Ricker, G. ; Lamb, D. ; Atteia, J. L. ; Kawai, N. / Are short GRBs really hard?. AIP Conference Proceedings. Vol. 836 2006. pp. 43-47
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AU - Sakamoto, T.

AU - Barbier, L.

AU - Barthelmy, S.

AU - Cummings, J.

AU - Fenimore, E.

AU - Gehrels, N.

AU - Hullinger, D.

AU - Krimm, H.

AU - Markwardt, C.

AU - Palmer, D.

AU - Parsons, A.

AU - Sato, G.

AU - Tueller, J.

AU - Aptekar, R.

AU - Cline, T.

AU - Golenetskii, S.

AU - Mazets, E.

AU - Pal'Shin, V.

AU - Ricker, G.

AU - Lamb, D.

AU - Atteia, J. L.

AU - Kawai, N.

PY - 2006/5/19

Y1 - 2006/5/19

N2 - Thanks to the rapid position notice and response by HETE-2 and Swift, the X-ray afterglow emissions have been found for four recent short gamma-ray bursts (GRBs; GRB 050509b, GRB 050709, GRB 050724, and GRB 050813). The positions of three out of four short GRBs are coincident with galaxies with no current or recent star formation. This discovery tightens the case for a different origin for short and long GRBs. On the other hand, from the prompt emission point of view, a short GRB shows a harder spectrum comparing to that of the long duration GRBs according to the BATSE observations. We investigate the prompt emission properties of four short GRBs observed by Swift/BAT. We found that the hardness of all four BAT short GRBs is in between the BATSE range for short and long GRBs. We will discuss the spectral properties of short GRBs including the short GRB sample of Konus-Wind and HETE-2 to understand the hard nature of the BATSE short GRBs.

AB - Thanks to the rapid position notice and response by HETE-2 and Swift, the X-ray afterglow emissions have been found for four recent short gamma-ray bursts (GRBs; GRB 050509b, GRB 050709, GRB 050724, and GRB 050813). The positions of three out of four short GRBs are coincident with galaxies with no current or recent star formation. This discovery tightens the case for a different origin for short and long GRBs. On the other hand, from the prompt emission point of view, a short GRB shows a harder spectrum comparing to that of the long duration GRBs according to the BATSE observations. We investigate the prompt emission properties of four short GRBs observed by Swift/BAT. We found that the hardness of all four BAT short GRBs is in between the BATSE range for short and long GRBs. We will discuss the spectral properties of short GRBs including the short GRB sample of Konus-Wind and HETE-2 to understand the hard nature of the BATSE short GRBs.

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