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The Supernova/GRB Connection

Published online by Cambridge University Press:  19 September 2016

P. Höflich ,
D. Baade ,
A. Khokhlov ,
L. Wang  and
J.C. Wheeler
P. Höflich
Affiliation:
Dept. of Astronomy, University of Texas, Austin, TX 78681, USA; [email protected]&, [email protected]
D. Baade
Affiliation:
ESO, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany; [email protected]
A. Khokhlov
Affiliation:
Naval Research Lab, Washington DC, USA; [email protected]
L. Wang
Affiliation:
Lawrence Berkeley Lab, CA 94720, USA; [email protected]
J.C. Wheeler
Affiliation:
Dept. of Astronomy, University of Texas, Austin, TX 78681, USA; [email protected]&, [email protected]

Summary

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We discuss the possible connection between supernova explosions (SN) and gamma-ray bursters (GRB) from the perspective of our current understanding of SN physics. Core collapse supernovae (SN) are the final stages of stellar evolution in massive stars during which the central region collapses, forms a neutron star (NS) or black hole, and the outer layers are ejected. Recent explosion scenarios assumed that the ejection is due to energy deposition by neutrinos into the envelope but detailed models do not produce powerful explosions. There is new and mounting evidence for an asphericity and, in particular, for axial symmetry in several supernovae which may be hard to reconcile within the spherical picture. The 3-D signatures are a key to understand core collapse supernovae and the GRB/SN connection. In this paper we study the effects and observational consequences of asymmetric explosions.

Type
Part VI Supernova and Gamma-Ray Burst Connections
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 403 - 410
Copyright
Copyright © Springer-Verlag 2005

References

1. Bisnovatyi-Kogan, G.S.: Sov. Astron. 14, 652 (1971)Google Scholar
2. Bowers, R.L. R.L., Wilson, J.R.: J.R. Astrophys. J. Suppl. 50, 115 (1982)Google Scholar
3. Colella, P., Woodward, P.R.: J. Comprit. Phys. 54, 174 (1984)CrossRefGoogle Scholar
4. Cropper, M. et al.: Mon. Not. R. Astron. Soc. 231, 685 (1988)Google Scholar
5. Fesen, R.A., Gunderson, K.S.: Astrophys. J. 470, 967 (1996)CrossRefGoogle Scholar
6. Gal-Yam, A., Shemmer, O., Dann, J.: IAUC 7811 (2002)Google Scholar
7. Höflich, P.: Pub. Astron. Soc. Paific 7, 434 (1988)CrossRefGoogle Scholar
8. Höflich, P.: Astron. Astrophys. 246, 481 (1991)Google Scholar
9. Höflich, P.: Astrophys. J. 443, 89 (1995)Google Scholar
10. Höflich, P., Wheeler, J.C., Hines, D., Trammell, S.: Astrophys. J. 459, 307 (1995)Google Scholar
11. Höflich, P., Khokhlov, A., Wang, L.: In: 20th Texas Conf. on Rei. Astro. (AIP Conf. Proc. 586 2001), p. 459 Google Scholar
12. Höflich, P.: astro-ph 0207103 (2002)Google Scholar
13. Hughes, J.P., Rakowski, C.E., Burrows, D.N., Slane, P.O.: Astrophys. J. Lett. 528 L109 (2000)Google Scholar
14. Jeffrey, D.J.: Astrophys. J. 375, 264 (1991)Google Scholar
15. Kinugasa, K. et al.: IAUC 7811 (2002)Google Scholar
16. Khokhlov, A.M.: J. Comput. Phys. 143, 519 (1998)Google Scholar
17. Khokhlov, A., Höflich, P., Oran, E., Wheeler, C., Wang, L.: Astrophys. J. Lett. 524 L107 (1999)Google Scholar
18. LeBlanc, J.M., Wilson, J.R.: Astrophys. J. 161, 541 (1970)Google Scholar
19. Leonard, D.C., Filippenko, A.V., Barth, A.J., Matheson, T.: Astrophys. J. 536, 239 (2000)Google Scholar
20. Lucy, L.B.: In: 4th Mason Conference, ed. Kafatos, M. (Cambridge Univ. Press: Cambridge 1998) p. 323 Google Scholar
21. Meikle, P. et al.: IAUC 7811 (2002)Google Scholar
22. Mendez, R.H. et al.: Astrophys. J. 334, 295 (1998)Google Scholar
23. Mönchmeyer, R., Schäfer, G., Müller, E., Kates, R.E.: Astron. Astrophys. 246, 417 (1991)Google Scholar
24. Schaefer, B.E. et al.: Astrophys. J. 588, 387 (2003)Google Scholar
25. Stanek, K.Z. et al.: Astrophys. J. Lett. 591 L17 (2003)Google Scholar
26. Straniero, O., Chieffi, A., Limongi, M.: Astrophys. J. 490, 425 (1997)Google Scholar
27. Strom, R., Johnston, H.M., Verbunt, F., Aschenbach, B.: Nature 373, 587 (1995)Google Scholar
28. Symbalisty, E.M.D.: Astrophys. J. 285, 729 (1984)Google Scholar
29. Trammell, S., Hines, D., Wheeler, J.C.: Astrophys. J. 414, 21 (1993)Google Scholar
30. Wang, L., Wheeler, J.C., Li, Z., Clocchiatti, A.: Astrophys. J. 467, 435 (1996)Google Scholar
31. Wang, L., Howell, A., Höflich, P., Wheeler, J.C.: Astrophys. J. 550, 1030 (2001)Google Scholar
32. Wang, L., Baade, D., Höflich, P., Wheeler, J.C.: Astrophys. J. 592, 457 (2003)CrossRefGoogle Scholar
33. Wang, L. et al.: Astrophys. J. 591, 1100 (2003)Google Scholar
34. Woosley, S.E., MacFadyen, A.I.: Astron. Astrophys. Suppl. 138, 499 (1999)Google Scholar