HOME    |    BROWSE    |    SEARCH    |    SUBSCRIPTION   |    SUBMISSION    |    REGISTRATION

Quick Search:
Author: Title/Abstract: Vol./No: Page:
PTP Online Top > Supplement (2007) > No.169
| Next Article >

Prog. Theor. Phys. Supplement No.169 (2007) pp. 7-11

[ Full Text PDF : FREE ACCESS (311K) ]

Diversity of the GRB-Supernova Connection: X-Ray-Flash SNe and Non-SN GRBs

Ken'ichi Nomoto,1 Nozomu Tominaga,1 Masaomi Tanaka,1 Keiichi Maeda2 and Tomoharu Suzuki1

1Department of Astronomy, University of Tokyo, Tokyo 113-0033, Japan
2Department of Earth Science and Astronomy, College of Arts and Science,
University of Tokyo, Tokyo 153-8902, Japan

Abstract:

Among the diversity of the connection between the long Gamma Ray Bursts (GRBs) and Supernovae (SNe), we present the models for the following two cases. (a) XRF-SN: we estimate the mass of the progenitor of SN 2006aj associated with X-Ray Flash 060218 is small enough to form a neutron star rather than a black hole. (b) Non-SN GRB: Two nearby long GRBs were not associated with SNe. Such “dark HNe” have been predicted in order to explain the origin of C-rich (hyper) metal-poor stars. We will show our attempt to explain the diversity in a unified manner with the jet-induced explosion model.


URL : http://ptp.ipap.jp/link?PTPS/169/7/
DOI : 10.1143/PTPS.169.7

[ Full Text PDF : FREE ACCESS (311K) ] Citation:

References:

  1. K. Nomoto et al., in Swift and GRBs: Unveiling the Relativistic Universe, ed. G. Chincarini et al., in press; astro-ph/0702472[e-print arXiv].
  2. S. Campana et al., Nature 442 (2006), 1008.
  3. E. Pian et al., Nature 442 (2006), 1011.
  4. M. Modjaz et al., Astrophys. J. 645 (2006), L21[IoP STACKS].
  5. P. A. Mazzali et al., Astrophys. J. 572 (2002), L61[IoP STACKS].
  6. P. A. Mazzali et al., Nature 442 (2006), 1018[CrossRef].
  7. M. Hamuy, Astrophys. J. 582 (2003), 905[IoP STACKS].
  8. K. Nomoto et al., Nature 371 (1994), 227[CrossRef].
  9. N. Tominaga, H. Umeda and K. Nomoto, Astrophys. J. 660 (2007), in press; astro-ph/0701381[e-print arXiv].
  10. N. Gehrels et al., Nature 444 (2006), 1044.
  11. J. P. U. Fynbo et al., Nature 444 (2006), 1047.
  12. M. Della Valle et al., Nature 444 (2006), 1050[CrossRef].
  13. A. Gal-Yam et al., Nature 444 (2006), 1053.
  14. N. Tominaga, K. Maeda, H. Umeda, K. Nomoto, M. Tanaka, N. Iwamoto, T. Suzuki and P. A. Mazzali, Astrophys. J. 657 (2007), L77[IoP STACKS].
  15. K. Maeda and K. Nomoto, Astrophys. J. 598 (2003), 1163[IoP STACKS].
  16. S. Nagataki, A. Mizuta and K. Sato, Astrophys. J. 647 (2006), 1255[IoP STACKS].
  17. L. Amati, M. Della Valle, F. Frontera, D. Malesani, C. Guidorzi, E. Montanari and E. Pian, Astron. Astrophys. (2007), submitted; astro-ph/0607148[e-print arXiv].
  18. K. Maeda and N. Tominaga, Astrophys. J. (2007), submitted.
  19. C. D. Bailyn, R. K. Jain, P. Coppi and J. A. Orosz, Astrophys. J. 499 (1998), 367[IoP STACKS].
  20. J. Tumlinson, Astrophys. J. 641 (2006), 1[IoP STACKS].
  21. R. Cayrel et al., Astron. Astrophys. 416 (2004), 1117.
  22. E. Depagne et al., Astron. Astrophys. 390 (2002), 187.
  23. N. Christlieb et al., Nature 419 (2002), 904[CrossRef].
  24. M. S. Bessell and N. Christlieb, in From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution, ed. V. Hill, P. François and F. Primas 228 (2005), 237.
  25. A. Frebel et al., Nature 434 (2005), 871[CrossRef].

[PTP HOME] [BROWSE] [SEARCH] [SUBSCRIPTION] [SUBMISSION] [REGISTRATION]

Copyright © Progress of Theoretical Physics 2013 All rights reserved.