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    • 1. The Death of Stars II: High Mass Stars
    ... Supernovae . Synthesis of Heavy Nuclei . Supernova Remnants (SNRs) . Hypernovae . Neutron Stars & Pulsars . Black Holes. ... Called hypernova e these are thought to occur when very massive stars undergo core collapse. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/stellarevolution_deathhigh.html -- 71.3 Кб -- 11.04.2016
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    2. http://www.atnf.csiro.au/research/Astro2010/talks/ferrario.pdf
    ... With P ~ 1 ms, Erot= I 2 /2 ~ 3x1052 erg and magnetars should power hypernovae (T. Thompson et al. 2004). ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/ferrario.pdf -- 1130.3 Кб -- 16.06.2010
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    3. Exotics I
    ... The -ray luminosity was about 10 41 J. Ron remarked that there had been a suggestion by Paczynski a few years ago postulating that GRBs could be the result of hypernovae, so this was one case where theory might have predicted the observation. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_1/dwarkadas/paper/node6.html -- 54.4 Кб -- 08.04.2016
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    4. Stellar Evolution Links
    ... When supernovae go hyper: A mystery surrounds an exploding star describes the story behind the discovery of the first hypernovae and its linkage with GRBs. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/stellarevolution_links.html -- 65.9 Кб -- 11.04.2016
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    5. Links for Stars
    ... When supernovae go hyper: A mystery surrounds an exploding star describes the story behind the discovery of the first hypernovae and its linkage with GRBs. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/cosmicengine/stars_links.html -- 66.7 Кб -- 11.04.2016
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    6. Wavebands
    ... Gamma-ray . <0.01 nm . > 3 x 10 19 . hypernova, accretion disks around black holes . > 10 8 K . INTEGRAL , GLAST . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/wavebands.html -- 62.7 Кб -- 11.04.2016
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    7. http://www.atnf.csiro.au/pasa/17_1/dwarkadas/paper.pdf
    ... The -ray luminosity was about 1041 J. Ron remarked that there had been a suggestion by Paczynski a few years ago postulating that GRBs could be the result of hypernovae, so this was one case where theory might have predicted the observation. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/17_1/dwarkadas/paper.pdf -- 122.6 Кб -- 04.08.2000
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    8. http://www.atnf.csiro.au/the_atnf/annual_reports/2003/Chapter7.pdf
    ... Were PKS 2225-253 & MRC 2220-700 radio hypernovae? ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2003/Chapter7.pdf -- 208.2 Кб -- 12.07.2004
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    9. http://www.atnf.csiro.au/nca/WG2.3%20report.pdf
    ... of many of these extremely metal-poor and thus old stars is their very peculiar abundance pattern by solar standards, including enormous over-abundances of C, N, O and/or Mg, which may be the result of hypernovae in the very first generation of stars ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/nca/WG2.3%20report.pdf -- 2925.2 Кб -- 20.09.2005
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