IUE and TIRGO observations of the symbiotic star HBV 475

Details IUE and TIRGO observations of the symbiotic star HBV 475 IUE and TIRGO observations of the symbiotic star HBV 475

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248...81n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 81-93. Research supported by SNSF.

Astronomy and Astrophysics

Astronomy

8

Iue, Novae, Stellar Evolution, Symbiotic Stars, Emission Spectra, Line Spectra, Radio Astronomy, Stellar Models, Stellar Spectrophotometry

Scientific paper

IUE has observed the symbiotic star HBV 475 since 1979, and the TIRGO long-term IR survey has done so since 1986. The star displays a strikingly regular periodic variation in the fluxes of the emission lines and of their wavelength positions. Observational results are presented in conjunction with an outline of the spectroscopic evolution of this symbiotic nova. The physical characteristics of the system are derived.

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