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23por Woltjer, L“…Various models for cosmic-ray production involving different aspects of the supernova process are evaluated. The difficulties in theories which make pulsars the main source of cosmic rays are stressed. (4 refs).…”
Publicado 1978
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24por Abarzhi, Snezhana I., Hill, Desmon L., Naveh, Annie, Williams, Kurt C., Wright, Cameron E.“…Supernovae are explosions of stars and are a central problem in astrophysics. …”
Publicado 2022
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26por Ianni, A., Pagliaroli, G., Strumia, A., Torres, F.R., Villante, F.L., Vissani, F.“…We derive the event-by-event likelihood that allows to extract the complete information contained in the energy, time and direction of supernova neutrinos, and specify it in the case of SN1987A data. …”
Publicado 2009
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29“…In 1965 Fritz Zwicky proposed a class of supernovae that he called "Type V", described as "excessively faint at maximum." …”
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30por Mobberley, Martin“…Supernovae represent the most violent stellar explosions in the universe. …”
Publicado 2007
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33“…We present a critical assessment of the SN1987A supernova cooling bound on axions and other light particles. …”
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34por Vink, Jacco“…Supernova remnants provide vital clues about the actual supernova explosions from X-ray spectroscopy of the supernova material, or from the imprints the progenitors had on the ambient medium supernova remnants are interacting with - all of which the author discusses in great detail. …”
Publicado 2020
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39“…We show that GRB 020405 was associated with a 1998bw-like supernova (SN) at the GRB's redshift which appeared dimmer and red relative to SN1998bw because of extinction in the host and our Galaxy. …”
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40“…The relative proximity of the recent gamma ray burst (GRB) 030329 resulted in a large gamma-ray fluence and in the brightest-ever afterglow (AG), hours after the burst, in the radio, optical and X-ray bands, permitting precise AG measurements, sensitive tests of models and an excellent occasion to investigate the association of GRBs with supernovae (SNe). The Cannonball (CB) model provides a good, simple and universal description of all AGs of GRBs of known redshift, so that it is straightforward to use it to predict what the expected SN signatures are. …”
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