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The early-type strong emission-line supergiants of the Magellanic Clouds : a spectroscopic zoology.
DOI: 10.1086/190945 Bibcode: 1984ApJS...55....1S

Shore, S. N.; Sanduleak, N.

The results of a spectroscopic survey of 21 early-type extreme emission line supergiants of the Large and Small Magellanic Clouds using IUE and optical spectra are presented. The combined observations are discussed and the literature on each star in the sample is summarized. The classification procedures and the methods by which effective temperat…

1984 The Astrophysical Journal Supplement Series
IUE 52
IUE observations of longitudinal and temporal variations in the Jovian auroral emission
DOI: 10.1086/161809 Bibcode: 1984ApJ...278..441S

Skinner, T. E.; Durrance, S. T.; Feldman, P. D. +1 more

The IUE's short wavelength spectrograph has been used to monitor the auroral emissions from Jupiter's northern hemisphere, yielding eight observations between January 1981 and January 1982 of H I Lyman-alpha and the H2 Lyman and Werner bands. Attention is given to an apparent periodic emission flux fluctuation, through detailed modeling of the emi…

1984 The Astrophysical Journal
IUE 52
The Be star phenomena. II - Spectral formation and structure of envelopes
Bibcode: 1984BASI...12..109H

Hirata, R.; Kogure, T.

The mechanisms of formation of the continuum and line spectra of Be stars and the morphology of their cool and hot envelopes are discussed in a review of recent theoretical and observational studies, supplementing the statistical evaluation of Kogure and Hirata (1982). Topics examined include the rapid rotation of Be stars, envelope dynamics, radi…

1984 Bulletin of the Astronomical Society of India
IUE 51
Stellar chromospheres and coronae in the Ursa Major cluster stars.
DOI: 10.1086/162160 Bibcode: 1984ApJ...281..815W

Golub, L.; Linsky, J. L.; Simon, T. +2 more

IUE spectra of 18 proposed members of the Ursa Major Cluster and Einstein X-ray images of 11 of these stars are discussed. Thirteen stars, six in the nucleus and seven in the extended comoving stream, are probably true members of the UMa Cluster in that their bright ultraviolet and X-ray surface fluxes indicate youth. Four stars, one in the nucleu…

1984 The Astrophysical Journal
IUE 51
The detection of X-rays from nova MUSCAE 1983 with the EXOSAT satellite.
DOI: 10.1086/184391 Bibcode: 1984ApJ...287L..31O

Beuermann, K.; Krautter, J.; Oegelman, H.

Nova Muscae 1983, a fast classical nova, was discovered on January 18, 1983, by Liller (1983). The present investigation is concerned with a study of this star on the basis of X-ray observations which have been conducted with the low- and medium-energy detectors of the Exosat satellite on April 20, 1984. The measured data are combined with other m…

1984 The Astrophysical Journal
Exosat 50
The remarkavle kinematics of the WR wind-blown bubble RCW 58.
DOI: 10.1093/mnras/211.3.679 Bibcode: 1984MNRAS.211..679S

Smith, L. J.; Pettini, M.; Hartquist, T. W. +1 more

High resolution, high signal-to-noise ratio, ultraviolet, and optical observations of HD 96548, a WN8 star surrounded by the nebula RCW 58 which consists of stellar ejecta enclosed in a wind-blown bubble, are presented. The spectra exhibit blueshifted absorption components in a number of interstellar lines arising from a variety of ions. The veloc…

1984 Monthly Notices of the Royal Astronomical Society
IUE 50
PG 1012-029 : a high-excitation eclipsing cataclysmic variable.
DOI: 10.1086/161607 Bibcode: 1984ApJ...276..233P

Green, R. F.; Liebert, J.; Penning, W. R. +2 more

The paper presents a photometric and spectrophotometric analysis of a new eclipsing cataclysmic variable, PG 1012-029, with an orbital period of 3 hr 14 minutes 18.7 s. The eclipse depth reaches 1.9 mag, is rounded at minimum, and shows a prolonged egress 'shoulder', as found for UX UMa and some other eclipsing systems. The spectrum shows strong h…

1984 The Astrophysical Journal
IUE 50
Multispectral analysis in the UV, optical and IR of HDE 245770 = A 0535+26.
Bibcode: 1984A&A...141..279D

Giovannelli, F.; Hensberge, H.; Persi, P. +10 more

The characteristics of the Be/X-ray binary system HDE 245770/A0535+26 are examined from UV, visual, IR and X-ray data. A sequence of observations in the optical preceding an X-ray outburst is interpreted as the ejection of a shell by the Be primary. An evolutionary scenario is presented that produces a system like HDE 245770. An effective temperat…

1984 Astronomy and Astrophysics
IUE 49
High-resolution, far-ultraviolet study of beta Draconis (G2 Ib-II) : transition region structure and energy balance.
DOI: 10.1086/162358 Bibcode: 1984ApJ...283..731B

Jordan, C.; Stencel, R. E.; Linsky, J. L. +2 more

High-resolution far ultraviolet spectra of the star Beta Draconis have been obtained with the IUE satellite. The observations and emission line data from the spectra are presented, the interpretation of the emission line widths and shifts is discussed, and the implications are given in terms of atmospheric properties. The emission measure distribu…

1984 The Astrophysical Journal
IUE 48
IUE UV spectra of extragalactic H II regions. I. The catalogue and the atlas.
Bibcode: 1984A&AS...57..361R

Benvenuti, P.; Rosa, M.; Joubert, M.

More than 150 spectrograms of giant H II complexes in spiral, blue compact and irregular galaxies, excluding the Magellanic Clouds, obtained within the period March 1, 1978 and April 1, 1982 with the International Ultraviolet Explorer (IUE) in the wavelength range 1150 A to 3200 A are cataloged. Many of the observations are presented in graphic fo…

1984 Astronomy and Astrophysics Supplement Series
IUE 47