The ultraviolet/optical variability of PG 1553+11

Details The ultraviolet/optical variability of PG 1553+11 The ultraviolet/optical variability of PG 1553+11

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.303m&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 303-304 (SEE N89

Astronomy and Astrophysics

Astronomy

5

Bl Lacertae Objects, Iue, Spaceborne Astronomy, Ultraviolet Astronomy, Ultraviolet Spectra, Variability, Visible Spectrum, Accretion Disks, Stellar Color, Stellar Luminosity

Scientific paper

Ultraviolet optical observations of the BL Lacertae object, PG 1553+11,
indicate that significant color variations are associated with the
luminosity variations seen in the ultraviolet and the optical regions of
the spectrum. The color variations are consistent with the presence of
an accretion disk in this system.

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