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- W1981846469 abstract "A series of low-dispersion spectra and one high-dispersion spectrum have been obtained of the catacylsmic variable CPD-48 deg 1577. Like other UX UMa stars, this variable exhibits the flat continuum of a luminous, thick, steady state accretion disk dominating its light from the far UV to the infrared. A wind mass loss rate of less than about 10 to the -9th solar mass/yr and an accretion rate of roughly 5 x 10 to the -9th solar mass/yr is roughly consistent with the range which characterizes other UX UMa stars. An SWP echelle spectrum reveals detailed line profile information on the N V, Si IV, and C IV resonance lines. He II 1640 A is remarkably weak and even absent in two of the spectra. The known properties and evolutionary status of CPD-48 deg 1577 and the other UX UMa stars are summarized." @default.
- W1981846469 created "2016-06-24" @default.
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- W1981846469 date "1985-05-01" @default.
- W1981846469 modified "2023-09-27" @default.
- W1981846469 title "On the nature of the UX Ursa Majoris-type nova-like variables - CPD-48 deg 1577" @default.
- W1981846469 doi "https://doi.org/10.1086/163192" @default.
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