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Optical spectra of dzeta Aurigae systems. IV. The January 1990 eclipse ofHR 2554 : detection of chomospheric absorption and extended plasma at 10 5 K.
Bibcode: 1992A&A...257..219S

Schroeder, K. -P.; Huensch, M.

Eclipse observations of HR 2554 are presented. These observations were obtained simultaneously during the January 1990 eclipse with ESO telescopes and the IUE satellite. Chromospheric absorption and changes in the circumstellar matter were investigated. Improved system parameters were derived from the light curve. For each of the composite spectra…

1992 Astronomy and Astrophysics
IUE 18
HIPPARCOS great-circle reduction - Theory, results and intercomparisons
Bibcode: 1992A&A...258...60V

van der Marel, Hans; Petersen, Carsten

In this paper some of the results of the great-circle reduction in the two data reduction consortia (NDAC and FAST) are presented. It is shown that the root-mean-square (rms) error of the great-circle abscissa of stars brighter than 10 mag is between 3-5 milli-arcsec. This is as was expected before launch, even in spite of the fact that the data-s…

1992 Astronomy and Astrophysics
Hipparcos 18
IUE observations of H Lyman-α in comet P/Giacobini-Zinner
DOI: 10.1016/0019-1035(92)90132-Q Bibcode: 1992Icar...97..260C

Feldman, Paul D.; Combi, Michael R.

Comet P/Giacobini-Zinner (1985 XIII) was observed during the flyby of the International Cometary Explorer (ICE) satellite and during the 3 preceding months by the International Ultraviolet Explorer (IUE) satellite. Models for the hydrogen abundance and spatial distribution, which were previously used to reproduce the observed spatial distribution …

1992 Icarus
IUE 18
The interrelation of UV and optical activity diagnostics in HK Lacertae.
DOI: 10.1093/mnras/259.2.302 Bibcode: 1992MNRAS.259..302O

Houdebine, E. R.; Butler, C. J.; Olah, K. +3 more

The study examines and compares optical photometric and UV (IUE) spectroscopic data on the active RS CVn star HK Lac gathered in the years 1979, 1980, and 1987. The photometry is modeled by representations of 'starspots' and, in general, it is found that the UV emission lines are stronger at times of spot maximum. The variable interstellar absorpt…

1992 Monthly Notices of the Royal Astronomical Society
IUE 18
Predictions of the solar wind interaction with Comet Grigg-Skjellerup
DOI: 10.1029/92GL00639 Bibcode: 1992GeoRL..19..837H

Coates, A. J.; Johnstone, A. D.; Huddleston, D. E.

The planned encounter of the Giotto spacecraft with comet Grigg-Skjellerup on 10th July 1992 promises to extend our knowledge of the solar wind interaction with comets substantially. While there have been spacecraft missions to comets before now, this mission is exploratory in the sense that the target comet is much older and therefore it has a mu…

1992 Geophysical Research Letters
Giotto 18
An Overview of Energetic Particle Measurements in the Jovian Magnetosphere with the EPAC Sensor on Ulysses
DOI: 10.1126/science.257.5076.1553 Bibcode: 1992Sci...257.1553K

Krupp, N.; Woch, J.; Keppler, E. +5 more

Observations of ions and electrons of probable Jovian origin upstream of Jupiter were observed after a corotating interplanetary particle event. During the passage of Ulysses through the Jovian bow shock, magnetopause, and outer magnetosphere, the fluxes of energetic particles were surprisingly low. During the passage through the "middle magnetosp…

1992 Science
Ulysses 18
X-ray observations of flat spectrum radio sources with the HEAO-A, Einstein and EXOSAT observatories.
Bibcode: 1992A&AS...96..339B

Pietsch, W.; Schaaf, R.; Witzel, A. +3 more

This paper presents X-ray data collected with the satellites HEAO-A, EINSTEIN (HEAO-B) and EXOSAT for flat spectrum radio sources. Most of the sources are from a complete sample of the high-declination 5 GHz survey.

1992 Astronomy and Astrophysics Supplement Series
Exosat 18
The hot subdwarf in the eclipsing binary HD 185510.
DOI: 10.1093/mnras/258.1.64 Bibcode: 1992MNRAS.258...64J

Simon, Theodore; Jeffery, C. S.; Evans, T. L.

High-resolution spectroscopic measurements of radial velocity are employed to characterize the eclipsing binary HD 185510 in terms of masses and evolutionary status. The IUE is used to obtain the radial velocities which indicate a large mass ratio Mp/Ms of 7.45 +/- 0.15, and Teff is given at 25,000 +/- 1000 K based on Ly alpha and UV spectrophotom…

1992 Monthly Notices of the Royal Astronomical Society
IUE 17
Spectroscopic binary orbits from ultraviolet radial velocities. Paper 10: CW Cephei (HD 218066)
Bibcode: 1992Obs...112..277S

Stickland, D. J.; Koch, R. H.; Pfeiffer, R. J.

Observations of CW Cephei were carried out repeatedly in the course of three days in December 1991, using the high-resolution, short-wavelength spectrograph of IUE, with an additional spectrum taken on February 6, 1992. The paper presents a log of these observations, which represent the only high-resolution observations of this star in the archive…

1992 The Observatory
IUE 17
Binary Star Observations With the Hubble Space Telescope Fine Guidance Sensors. II. Bright Hyades
DOI: 10.1086/116051 Bibcode: 1992AJ....103..190F

Franz, O. G.; Nelan, E.; Lattanzi, M. G. +3 more

The paper reports on astrometric measurements performed with the Hubble Space Telescope fine guidance sensors in the transfer scan mode on selected bright member stars of the Hyades cluster. The purpose of these measurements was to quickly validate this mode of operation of the fine guidance sensors - in the presence of many optical anomalies - an…

1992 The Astronomical Journal
eHST 17