Search Publications

The partial phase of the eclipse of Epsilon Aurigae.
DOI: 10.1086/184046 Bibcode: 1983ApJ...269L..17C

Kondo, Y.; Stencel, R. E.; Chapman, R. D.

Ultraviolet spectra of the peculiar eclipsing binary Epsilon Aurigae (FO Ia + ?) were obtained with the International Ultraviolet Explorer at pre-eclipse and ingress partial phases. The results show a wavelength dependence of the eclipse in contrast to the grayness (non-wavelength dependence) of the eclipse observed in visible light. From the curr…

1983 The Astrophysical Journal
IUE 17
The enigmatic composite system HD 45166 - B8V +qWR or SdO ?
DOI: 10.1093/mnras/203.3.619 Bibcode: 1983MNRAS.203..619W

Willis, A. J.; Stickland, D. J.

High- and low-resolution IUE ultraviolet spectroscopic observations of the binary system HD 45166, previously classified as qWR + B8 V, obtained at several epochs are presented. The UV spectra show a photospheric absorption spectrum from highly ionized species like Fe v, which with the observation of B8 V absorptions in the visible, confirms the b…

1983 Monthly Notices of the Royal Astronomical Society
IUE 17
The UV spectrum of the BL Lac object PKS 0521-36.
DOI: 10.1093/mnras/203.2.565 Bibcode: 1983MNRAS.203..565D

Maraschi, L.; Tanzi, E. G.; Treves, A. +3 more

Ultraviolet observations (1200-3000 Å) with the IUE satellite of the BL Lac object PKS 0521-36 are presented. The only emission line which appears clearly in the spectrum is Lyα, which is asymmetric with a component displaced ≡3000 km s-1 to the red. The intensity of the line and the upper limits on other lines are compared with the mod…

1983 Monthly Notices of the Royal Astronomical Society
IUE 17
Observations of two peculiar emission objects in the Large MagellanicCloud.
DOI: 10.1086/161557 Bibcode: 1983ApJ...275..584K

Kafatos, M.; Stencel, R. E.; Michalitsianos, A. G. +1 more

Ultraviolet and visual wavelength spectra were obtained of two peculiar emission objects, Henize S63 and Sanduleak's star in the Large Magellanic Cloud. Previously not observed in the near- or far-ultraviolet, both objects exhibit strong permitted and semiforbidden line emissions. Estimates based on the absolute continuum flux of the hot companion…

1983 The Astrophysical Journal
IUE 17
HD 207739 : A strange composite star.
DOI: 10.1086/183937 Bibcode: 1983ApJ...264L..19P

Kondo, Y.; Holm, A. V.; Parsons, S. B.

This star, classified F8 IIe + B:, has a very unusual ultraviolet spectrum, with abnormally strong and numerous absorption features in the far-UV and exceptionally strong Mg II emission. There is some resemblance to shell and pre-main-sequence B stars, but it more closely matches the strange spectra of the eclipsing systems VV Cep and SX Cas, and …

1983 The Astrophysical Journal
IUE 17
Element identifications in the ultraviolet spectrum of HD 101065.
DOI: 10.1086/161327 Bibcode: 1983ApJ...272..646W

Stickland, D. J.; Byrne, P. B.; Wegner, G. +1 more

Ultraviolet spectroscopic observations with the IUE satellite of the controversial peculiar star HD 101065 are presented and discussed. Low-resolution spectra combined with published visual and infrared broad-band photometry show that the star's spectral energy distribution is greatly distorted, presumably by the severe line blanketing. However, t…

1983 The Astrophysical Journal
IUE 17
Simultaneous X-ray and ultraviolet observations of Epsilon Orionis and Kappa Orionis.
DOI: 10.1086/160945 Bibcode: 1983ApJ...268..205C

Dupree, A. K.; Cassinelli, J. P.; Hartmann, L. +2 more

Simultaneous observations were made with the Einstein Observatory, the International Ultraviolet Explorer, and the Copernicus satellite of the supergiant stars η Ori (B0 Ia) and κ Ori (B0.5 Ia). The X-ray observations spanned periods of 7 hours and 10 hours, and the ultraviolet observations spanned 15 and 18 hours for ηOri and κ Ori, respectively.…

1983 The Astrophysical Journal
IUE 16
Interstellar absorption lines in the spectrum of 3C 273.
DOI: 10.1086/161431 Bibcode: 1983ApJ...274..136Y

York, D. G.; Cowie, L. L.; Blades, J. C. +3 more

Absorption lines near the rest wavelengths of the Si IV doublet (wavelengths 1393.76, 1402.77) with equivalent widths 533 and 235 mA are reported in the spectrum of QSO 3C 273. The profiles show the nature of hot gas along a high-latitude (b = 64 deg) line of sight through our entire halo. The lines have full width at half-maxima of 100 km/s, comp…

1983 The Astrophysical Journal
IUE 16
A multiwavelength study of the short-period cataclysmic variable V442 Ophiuchi.
DOI: 10.1086/131200 Bibcode: 1983PASP...95..509S

Szkody, P.; Shafter, A. W.

The results of a program of observations of the cataclysmic variable V442 Oph from UV to IR wavelengths are reported. The observations comprise IUE SWP and LWR-camera spectra from October, 1981; UBVr and R photometry at Manastash Ridge Observatory from August, 1980; UBV photometry and IR measurements at Kitt Peak from July, 1981; and Coudespectros…

1983 Publications of the Astronomical Society of the Pacific
IUE 15
IUE observations of E 1405-451 : a new AM Herculis type cataclysmic variable.
DOI: 10.1086/183974 Bibcode: 1983ApJ...266L..39N

Nousek, J. A.; Pravdo, S. H.

International Ultraviolet Explorer observations of the recently discovered AM Herculis type cataclysmic variable E1405-451 reveal a UV spectrum (1000-3000 A) similar to the other members of the type. The continuum flux distribution rises steeply at short wavelength and shows the effects of interstellar extinction. Best fit parameters for a blackbo…

1983 The Astrophysical Journal
IUE 15