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Optical and Near-IR Observations of SN 1998bw
Published online by Cambridge University Press: 19 September 2016
Abstract
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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
- Copyright
- Copyright © Springer-Verlag 2005
References
6.
Galama, T.J., Vreeswijk, P.M., Pian, E., Frontera, F., Doublier, V., Gonzalez, J.F.: IAUC
6895 (1998)Google Scholar
9.
Garnavich, P., Matheson, T., Olszewski, E.W., Harding, P., Stanek, K.Z.: IAUC
8108 (2003)Google Scholar
12.
Kay, L.E., Halpern, J.P., Leighly, K.M., Heathcote, S., Magalhaes, A.M.: IAUC
6969 (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
21.
Sollerman, J., Kozma, C., C., , Fransson, C., Leibundgut, B., Lundqvist, P., Ryde, F., Woudt, P.: Astrophys. J. Lett.
537, L127 (2000)Google Scholar