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  • 1
    Electronic Resource
    Electronic Resource
    Pulsar Ejection in Supernova Events (1970)
    [s.l.] : Nature Publishing Group
    Nature 228 (1970), S. 1072-1073 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Fowler and Hoyle3 suggested some time ago that the symmetric ejection of radio-luminous material from, galaxies could be caused by asymmetrical processes occurring in the collapse of very massive objects. Indeed, it is known that such an imploding system is Rayleigh-Taylor unstable. Thus the more ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/2281072a0
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    Is PSR1957 + 20 eclipsed by a comet, magnetosphere or particulate cloud? (1989)
    [s.l.] : Nature Publishing Group
    Nature 337 (1989), S. 236-238 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] PSR1957 + 20 consists of a 1.6-ms pulsar and a 0.02-Má© companion1. The eclipse duration (8 x 1010 cm of orbital trajectory for a pulsar mass of 1.4 Má© and therefore a separation a = 1.7 x 1011 cm), is more than a factor of two larger than the Roche-lobe distance (Lt is ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/337236a0
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  • 3
    Electronic Resource
    Electronic Resource
    Neutron star disk formation from supernova fall-back and possible observational consequences (1988)
    [s.l.] : Nature Publishing Group
    Nature 333 (1988), S. 644-645 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Let us take as a simple supernova model a sphere of matter that is set into expansion with a velocity directly proportional to distance from the centre. As long as density declines with distance from the centre, a sufficiently large velocity gradient leads to all of the mass beyond some value M0 ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/333644a0
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