Search Publications

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
The gravitational wave experiment
Bibcode: 1992A&AS...92..431B

Comoretto, G.; Giampieri, G.; Asmar, S. W. +6 more

Since the optimum size of a gravitational wave detector is the wave length, interplanetary dimensions are needed for the mHz band of interest. Doppler tracking of Ulysses will provide the most sensitive attempt to date at the detection of gravitational waves in the low frequency band. The driving noise source is the fluctuations in the refractive …

1992 Astronomy and Astrophysics Supplement Series
Ulysses 17
EXOSAT Observations of the Be/X-Ray Binary 4U 2206+54
DOI: 10.1086/172095 Bibcode: 1992ApJ...401..678S

Saraswat, Priyamvada; Apparao, Krishna M. V.

We present the X-ray observations of the Be star binary system 4U 2206 + 54 made with the EXOSAT satellite during the period 1983-1985. The observations were carried out on three occasions, each separated by roughly a year. The source was active during the 1983 and 1985 observations and several short duration flares were observed. The spectrum, du…

1992 The Astrophysical Journal
Exosat 16
Spatially Resolved Ultraviolet Spectroscopy of the Liner Galaxy NGC 3998
DOI: 10.1086/171105 Bibcode: 1992ApJ...387..536R

Filippenko, A. V.; Branduardi-Raymont, G.; Reichert, G. A. +3 more

We report results of recent IUE observations of the low-ionization nuclear emission-line region (LINER) galaxy NGC 3998. Spatial structure in the long-wavelength emission is apparent; the spatial profiles in the LWP images show a two-component structure, with an unresolved central component superposed on extended underlying emission. We have used …

1992 The Astrophysical Journal
IUE 16