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  • 1985-1989  (2)
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Material
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Year
  • 1
    Electronic Resource
    Electronic Resource
    BR Lupi: A new SU UMa-star (1987)
    Springer
    Astrophysics and space science 136 (1987), S. 247-250 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract From the presence of superhumps in its outburst light curve, the dwarf nova BR Lup is shown to be a member of the SU UMa sub-class of cataclysmic variables. Its orbital period is estimated to be 0.0789 d.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00642116
    Library Location Call Number Volume/Issue/Year Availability
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    Paper (German National Licenses)
    Fulltext
  • 2
    Electronic Resource
    Electronic Resource
    BV centauri: dwarf or classical nova? (1986)
    Springer
    Astrophysics and space science 122 (1986), S. 73-80 
    Details
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The similarity in properties of GK Per and BV Cen suggests that the latter may be a classical nova remnant rather than a dwarf nova. Our Hα and V CCD photometry show no sign of a nova shell but disclose the presence of a close and probably physical companion. BV(RI) c CCD photometry of the companion, assumed to be a dwarf, givesM v =3.1±0.3 for BV Cen at quiescence. Even though half of the light in BV Cen comes from the secondary this is much brighter than expected for a dwarf nova and supports the conclusion that BV Cen was an unrecorded nova.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00654382
    Library Location Call Number Volume/Issue/Year Availability
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    Paper (German National Licenses)
    Fulltext
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