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  • 1
    Electronic Resource
    Electronic Resource
    Magnetic Fields of Degenerate Stars (1992)
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 30 (1992), S. 143-184 
    Details
    ISSN: 0066-4146
    Source: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1146/annurev.aa.30.090192.001043
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  • 2
    Electronic Resource
    Electronic Resource
    Superfluidity in neutron stars
    Amsterdam : Elsevier
    Physics Letters A 39 (1972), S. 285-286 
    Details
    ISSN: 0375-9601
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
    URL: http://linkinghub.elsevier.com/retrieve/pii/0375-9601(72)90992-9
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  • 3
    Electronic Resource
    Electronic Resource
    Ultrahigh Energy Gamma Rays and Cosmic Rays from Accreting Degenerate Stars (1986)
    Oxford, UK : Blackwell Publishing Ltd
    Annals of the New York Academy of Sciences 470 (1986), S. 0 
    Details
    ISSN: 1749-6632
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1749-6632.1986.tb47991.x
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  • 4
    Electronic Resource
    Electronic Resource
    Radio emission from cataclysmic variables (1987)
    Springer
    Astrophysics and space science 130 (1987), S. 53-68 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The study of radio emission from cataclysmic variables (CVs) is a new and developing field. Radio emission from novae, recurrent novae, dwart novae and each of the subclasses (AM Her and DQ Her) of magnetic CVs have now been reported and are reviewed here. These observations are shown to provide, in general, a probe of the structure of the CV on length scales typically ≳1011 cm. Radiation mechanisms, both incoherent and coherent, relevant to the observed radio emission are also discussed. These suggest that the red dwarf in AM Her and DQ Her is also magnetized and provides support for theories for the evolution of CVs which require a magnetized secondary star.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00654972
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  • 5
    Electronic Resource
    Electronic Resource
    Models for optical and infrared polarization from CW1103+254 (1987)
    Springer
    Astrophysics and space science 131 (1987), S. 657-663 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Multiband observations of the AM Herculis-type binary CW1103+254 show significant circular polarization (∼13%) in the J band. Recently, a model with high temperature (kT∼20 keV) and small dimensionless plasma parameter (∧∼104) was suggested for the emitting region. However, it gives negligible polarization in the J band. In this paper, a method, in which the J band polarization and the peak frequency ν⋆ of the spectrum are taken into account, is used to determine T and ∧. For the viewing angle θ=80° and the magnetic field B=30MG, we find that kT=5.0 keV and ∧=106. The temperature of the emitting region is close to the value (kT=8.7 keV) derived for the region emitting cyclotron lines in VV Puppis. If these radiations arise from the post-shock regions, then these temperatures are significantly lower than those predicted by standard accretion models or the shock structure is inhomogenous and more complex than previously assumed.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00668153
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  • 6
    Electronic Resource
    Electronic Resource
    Gamma-ray bursts from degenerate stars (1976)
    Springer
    Astrophysics and space science 42 (1976), S. 83-87 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract A number of models have been proposed for the observed cosmic gamma-ray bursts. A class of such models involves the use of magnetic energy as the principal source of energy required for the bursts. In this case, arguments are presented to show that degenerate stars are favored. Mechanisms for magnetohydrodynamic instabilities in white dwarfs and neutron stars are discussed. Preliminary work indicates that magnetic white dwarfs can (but neutron stars probably cannot) account for many of the observed features of the bursts.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00645529
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  • 7
    Electronic Resource
    Electronic Resource
    The search for a pulsar in supernova 1987A
    Amsterdam : Elsevier
    Endeavour 14 (1990), S. 61-65 
    Details
    ISSN: 0160-9327
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Natural Sciences in General
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1016/0160-9327(90)90073-Z
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  • 8
    Electronic Resource
    Electronic Resource
    Ultra-high energy γ rays and cosmic rays from accreting degenerate stars (1985)
    [s.l.] : Nature Publishing Group
    Nature 313 (1985), S. 767-768 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Cyg X-3 is a remarkable X-ray source3, emitting X rays of energy ?1 keV, with a luminosity 3 xl038 erg s-1, which are modulated with a 4.8-h period, thought to be the orbital period of the underlying binary-star system (though there is no direct spectroscopic evidence to support this conclusion). ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/313767a0
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  • 9
    Electronic Resource
    Electronic Resource
    Initial spin and magnetic field of the fast pulsar 4C21.53 (1983)
    [s.l.] : Nature Publishing Group
    Nature 302 (1983), S. 124-125 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] A remarkable feature of pulsars is that despite their compact sizes (radii jR106cm) their angular momenta are much less than that of their progenitors on the main sequence. Furthermore, they are slow rotators in the sense that u)2R3/GM" 1, where ? is the angular velocity and M == IM its mass. Note ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/302124a0
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  • 10
    Electronic Resource
    Electronic Resource
    Pulsar formation (1989)
    [s.l.] : Nature Publishing Group
    Nature 338 (1989), S. 712-712 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] SIRá€"Lindley1 states that the report2 3 of a half-millisecond pulsar in the remnant of supernova 1987A "has surprised everybody and could, if confirmed, stand theory on its head". He has apparently overlooked several papers (refs 4 and 5, for example) suggesting that pulsars may ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/338712c0
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