New results on PU VUL

Details New results on PU VUL New results on PU VUL

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..305f&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 305-308 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

11

Infrared Radiation, Stellar Spectra, Ultraviolet Radiation, Variable Stars, Emission Spectra, Iue, Stellar Luminosity

Scientific paper

The authors analyze coordinated UV and IR observations of the nova-like
variable PU Vul made during the 1983 September active phase. A reddening
of E(B-V) = 0.49 is obtained, while the 1980 fading is attributed to
absorption by dust formed in the interactive binary system, containing
an active warm component and an M giant.

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