Search Publications

High luminosity X-ray binaries: IUE results
DOI: 10.1016/0273-1177(82)90257-5 Bibcode: 1982AdSpR...2i..75H

Hutchings, J. B.

The contribution of UV spectroscopy to the understanding of massive X-ray binaries, is reviewed. Results are given in the context of normal stars and binaries. The IUE results have enabled a greater understanding of the effects of accretion disks and X-ray heating in the systems, and provide absolute fluxes and luminosities. High-dispersion data r…

1982 Advances in Space Research
IUE 1
Erratum - Ground-Based and IUE Spectral Observations of Au-Monocerotis
DOI: 10.1086/131077 Bibcode: 1982PASP...94..872S

Sahade, J.; Ferrer, O. E.

1982 Publications of the Astronomical Society of the Pacific
IUE 1
The early-type component in nu.01 Sgr.
DOI: 10.1086/131037 Bibcode: 1982PASP...94..647K

Kondo, Y.; McCluskey, G. E.; Wu, C. -C.

Four low-resolution UV spectra of v1 Sgr (cK2) were obtained with the IUE satellite to investigate the nature of the hot component in this object, which was detected in the Astronomical Netherlands Satellite UV photometric data. The IUE results show that the spectral energy distribution of v1 Sgr in the FUV is comparable to that of a B9 star. FUV …

1982 Publications of the Astronomical Society of the Pacific
IUE 1
Determination of the rotational excitation temperature in solar type stars.
DOI: 10.1007/BF00648909 Bibcode: 1982Ap&SS..87...81F

Rego, M.; Fernandez-Figueroa, M. J.; Perea, A.

The OH molecular spectrum has been identified in three solar type stars, β Com, β CVn, and κ Cet. The rotational excitation temperature from molecular line intensities of OH has been determined for these stars. The observations in high resolution were made by use of the IUE satellite.

1982 Astrophysics and Space Science
IUE 1
IUE and Einstein observations of supernovae
DOI: 10.1016/0273-1177(82)90254-X Bibcode: 1982AdSpR...2i..51P

Palumbo, G. G. C.

In this paper IUE observations of two type II and three type I Supernovae (see Table I and Table II) are reviewed. The type II events were also observed by Einstein and SN 1980k was detected in the soft X-ray energy band. Combining UV spectra available of the same events one has the elements to construct a physical picture which accounts for all o…

1982 Advances in Space Research
IUE 1
The coronas of galaxies
DOI: 10.1038/scientificamerican0882-54 Bibcode: 1982SciAm.247b..54D

Savage, B. D.; de Boer, K. S.

The instrumentation and results of observations of interstellar and intergalactic gases are reviewed, particularly for UV satellite data on the dynamics and composition of the galactic corona. Radio telescopes began the mapping of gas in the central galactic disk in the 1950's, using 21-cm readings to detect atomic hydrogen clouds 100,000 light ye…

1982 Scientific American
IUE 0
IUE Observatory - European Space Agency - Villafranca Satellite Tracking Station / Vilspa
Bibcode: 1982QJRAS..23..123P

Penston, M. V.; Heck, A.

1982 Quarterly Journal of the Royal Astronomical Society
IUE 0
Observations de comètes faibles avec IUE.
Bibcode: 1982LAstr..96..299F

Festou, M.

Spectral observations of eight comets, including seven periodic comets, made in the range 1150-3400 A with the IUE satellite are presented. Comet Bradfield, the sole nonperiodic comet observed, is found to exhibit strong OH and atomic hydrogen emissions from the decomposition of water, along with oxygen, carbon, sulfur, carbon disulfide, C2 and CO…

1982 L'Astronomie
IUE 0
The thermonuclear model for X-ray transients.
Bibcode: 1982ApJ...258..595W

Woosley, S. E.; Weaver, T. A.; Wallace, R. K.

1982 The Astrophysical Journal
IUE 0
IUE observations of cataclysmic variables
DOI: 10.1016/0273-1177(82)90261-7 Bibcode: 1982AdSpR...2i..99S

Szkody, P.

The four years of IUE operation have revealed that the ultraviolet region of the spectrum contributes a dominant share of the emerging energy from cataclysmic variables and provides important clues to the physical nature of these systems. The implications of the continuum flux distributions and line spectra for the determination of the accretion r…

1982 Advances in Space Research
IUE 0