Search Publications

HD 115781 and HD 116204—two RS CVn binaries
DOI: 10.1007/BF02715066 Bibcode: 1988JApA....9..213G

Fekel, Francis C.; Griffin, R. F.

HD 115781 and HD 116204 (BL CVn and BM CVn) are shown to be RS CVn binaries with periods near 20 days. HD 115781 is double-lined; the primary type is about K1III, while the secondary is probably a late-type subgiant. The masses of the two components are equal within observational error. There is substantial photometric variability with a period ha…

1988 Journal of Astrophysics and Astronomy
IUE 11
Ultraviolet Variability of HD62001 - the Central Star of the Missing Nebula VORONTSOV-VELYAMINOV1-7
DOI: 10.1007/BF02714193 Bibcode: 1983JApA....4...59R

Rao, N. K.; Gilra, D. P.

IUE observations of HD 62001 do not confirm the ultraviolet variability of 0.15 mag seen from the ANS observations. These intriguing variations in ANS observations seem to be caused by a nearby (∼ 70 arcsec away) B star getting in and out of the field of view of the telescope, which had a jitter of 20 arcsec. There seems to be no evidence for the …

1983 Journal of Astrophysics and Astronomy
IUE 0
Ultraviolet Observations of the Hydrogen Deficient Variable Star Mv-Sagittarii
DOI: 10.1007/BF02714565 Bibcode: 1982JApA....3...79R

Nandy, K.; Rao, N. K.

IUE observations of the hydrogen-deficient irregular variable star MV Sgr obtained in 1980 June-October and also in 1979 November are discussed. These observations show a prominent λ 2200 absorption feature. A value ofE(B — V) = 0.55 is deduced from the strength of λ 2200 band assuming that this absorption is caused by interstellar medium. The der…

1982 Journal of Astrophysics and Astronomy
IUE 7