Hostname: page-component-669899f699-g7b4s Total loading time: 0 Render date: 2025-04-27T01:36:24.036Z Has data issue: false hasContentIssue false
  • English
  • Français

Optical and Near-IR Observations of SN 1998bw

Published online by Cambridge University Press:  19 September 2016

Ferdinando Patat
Ferdinando Patat*
Affiliation:
European Southern Observatory, Garching, Germany; [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Thus, the observation of gamma-ray line emission from a young supernova seems very promising in the near future. The observation, or even a null observation at a low threshold, will give significance in the fields of nuclear astrophysics and supernova theory. The scientific importance of a positive measurement would be analogous with and comparable to the importance of successful detection of neutrinos from the Sun.

Clayton, Colgate, and Fishman [2].

Type
Part VI Supernova and Gamma-Ray Burst Connections
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 381 - 390
Copyright
Copyright © Springer-Verlag 2005

References

1. Bloom, J.S. et al.: Nature 401, 453 (1999)CrossRefGoogle Scholar
2. Clayton, D.D., Colgate, S.A., Fishman, G.J.: Astrophys. J. 155, 75 (1969)Google Scholar
3. Colgate, S.A.: Astrophys. J. 187, 333 (1974)Google Scholar
4. Filippenko, A.V.: IAUC 6969 (1998)Google Scholar
5. Fynbo, J.U. et al.: Astrophys. J. Lett. 542 L89 (2000)Google Scholar
6. Galama, T.J., Vreeswijk, P.M., Pian, E., Frontera, F., Doublier, V., Gonzalez, J.F.: IAUC 6895 (1998)Google Scholar
7. Galama, T.J. et al.: Nature 1395, 670 (1998)Google Scholar
8. Galama, T.J. et al.: Astron. Astrophys. Suppl. 138, 465 (1999)Google Scholar
9. Garnavich, P., Matheson, T., Olszewski, E.W., Harding, P., Stanek, K.Z.: IAUC 8108 (2003)Google Scholar
10. Höffich, P., Wheeler, J.C., Wang, L.: Astrophys. J. 521, 179 (1999)Google Scholar
11. Iwamoto, K. et al.: Nature 395, 672 (1998)CrossRefGoogle Scholar
12. Kay, L.E., Halpern, J.P., Leighly, K.M., Heathcote, S., Magalhaes, A.M.: IAUC 6969 (1998)Google Scholar
13. Kulkarni, S.R. et al.: Nature 395, 663 (1998)Google Scholar
14. C.Lidman, Doublier, V., Gonzalez, J.F., Augusteijn, T., Hainaut, O., Boehn-hardt, H., Patat, F., Leibundgut, B.: IAUC 6895 (1998)Google Scholar
15. Mazzali, P.A., Iwamoto, K., Nomoto, K.: Astrophys. J. 545, 407 (2000)Google Scholar
16. McKenzie, E.H., Schaefer, B.E.: Pub. Astron. Soc. Pacific 111, 964 (1999)CrossRefGoogle Scholar
17. Patat, F., Piemonte, A.: IAUC 6918 (1998)Google Scholar
18. Patat, F. et al.: Astrophys. J. 555, 900 (2001)Google Scholar
19. Pian, E. et al.: Astron. Astrophys. Suppl. 138, 463 (1999)Google Scholar
20. Soffita, P. et al.: IAUC 6884 91998)Google Scholar
21. Sollerman, J., Kozma, C., C., , Fransson, C., Leibundgut, B., Lundqvist, P., Ryde, F., Woudt, P.: Astrophys. J. Lett. 537, L127 (2000)Google Scholar
22. Sollerman, J. et al.: Astron. Astrophys. 386, 944 (2002)CrossRefGoogle Scholar
23. Stathakis, R.A. et al.: Mon. Not. R. Astron. Soc. 314, 807 (2000)CrossRefGoogle Scholar