Author:
Aglietta M.,Castellina A.,Fulgione W.,Trinchero G.,Vernetto S.,Castagnoli C.,Galeotti P.,Saavedra O.,Amaldi E.,Frasca S.,Pallottino G. V.,Pizzella G.,Rapagnani P.,Ricci F.,Astone P.,Cosmelli C.,Bassan M.,Coccia E.,Modena I.,Bonifazi P.,Castellano M. G.,Visco M.,Badino G.,Bologna G.,Dadykin V. L.,Khalchukov F. F.,Korolkova I. V.,Kortchaguin P. V.,Kudryatzev V. A.,Malguin A. S.,Ryassny V. G.,Ryazhskaya O. G.,Yakushev V. F.,Zatsepin G. T.,Gretz D.,Weber J.,Wilmot G.
Publisher
Springer Science and Business Media LLC
Reference11 articles.
1. The first optical observation of the SN1987A occurred at 10 h 40 min UT of Feb. 23 and the last observation of LMC without the supernova at 2h 13 min (E. J. Wampler et al.:Astron. Astrophys.,182, L51 (1987). All extrapolated light curves are dependent on the density distribution in the envelope of the pre supernova star.
2. M. Aglietta et al.: Proceedings of the Rencontres de Physique de la Vallée d'Aoste, La Thuile, edited byM. Greco (Frontières, 1988), p. 49;M. Aglietta et al.: Europhys. Lett.,3, 1315 (1987).
3. K. S. Hirata et al.:Phys. Rev. Lett.,58, 1490 (1987);K. S. Hirata et al.: Phys. Rev. D,38, 448 (1988).
4. R. M. Bionta et al.:Phys. Rev. Lett. 58, 1494 (1987).
5. E. M. Alexeyev et al.:Sov. JETP Lett. 45, 461 (1987).
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