Search Publications

Discrete wave packets at the proton cyclotron frequency at comet P/Halley
DOI: 10.1029/92GL02613 Bibcode: 1993GeoRL..20..153M

Neubauer, F. M.; Mazelle, C.

We present in this letter the first experimental evidence for wave packets near the local proton cyclotron frequency in the plasma environment of a comet. The observations have been made by the GIOTTO magnetometer experiment (MAG) around comet P/Halley on both sides of closest approach. The waves are always left-handed in the spacecraft frame, ell…

1993 Geophysical Research Letters
Giotto 51
On the nature of the blue light in central cluster galaxies.
DOI: 10.1093/mnras/265.2.431 Bibcode: 1993MNRAS.265..431C

Fabian, A. C.; Crawford, C. S.

An excess blue component of light, extended over the innermost few kpc, is observed in several central cluster galaxies. Using a combination of blue optical spectra and IUE data, we show that the spectrum of the excess blue light is consistent with both star formation dominated by the light of B5 stars, and power-law spectra with slopes between λ^…

1993 Monthly Notices of the Royal Astronomical Society
IUE 51
Saturn's Upper Atmospheric Hazes Observed by the Hubble Space Telescope
DOI: 10.1006/icar.1993.1183 Bibcode: 1993Icar..106..428K

Karkoschka, Erich; Tomasko, Martin G.

We observed Saturn with the Hubble Space Telescope at wavelengths 0.30-0.89 µm for the purpose of determining the distribution of hazes. In the stratosphere, haze optical depths in the ultraviolet are essentially zero for midnorthern latitudes, are small (∼0.2) at low latitudes and mid-southern latitudes, but large (almost unity) above 70° n…

1993 Icarus
eHST 50
Correlated variations of UV and radio emissions during an outstanding Jovian auroral event
DOI: 10.1029/93JE01802 Bibcode: 1993JGR....9818779P

Moos, H. W.; Bame, S. J.; Zarka, P. +6 more

An exceptional Jovian aurora was detected in the FUV on December 21, 1990, by means of Vilspa and Goddard Space Flight Center (GFSC) International Ultraviolet Explorer (IUE) observations. This event included intensification by a factor of three between December 20 and 21, leading to the brightest aurora identified in the IUE data analyzed, and, in…

1993 Journal of Geophysical Research
IUE Ulysses 50
PG 0308+096 and PG 1026+002: Two New Short Period Binary Stars Resulting From Common-Envelope Evolution
DOI: 10.1086/116569 Bibcode: 1993AJ....105.1945S

Green, Richard F.; Sion, Edward M.; Saffer, Rex A. +5 more

Ultraviolet spectroscopy, optical spectroscopy, and spectrophotometry have been used to study the excess UV stars PG 0308 + 096 and PG 1026 + 002. Both objects are short-period binary systems, each containing a DA white dwarf star and a dM star. Orbital periods of approximately 0.284 day for PG 0308 + 096, and aproximately 0.597 day for PG 1026, h…

1993 The Astronomical Journal
IUE 49
Spectral analysis of DY Centauri, a hot R Coronae Borealis star with an unusually high hydrogen content.
Bibcode: 1993A&A...270..167J

Heber, U.; Jeffery, C. S.

The photospheric parameters of DY Cen, an H-deficient early-B supergiant that is spectroscopically similar to the pulsating, extreme-He star BD-9 deg 4395, have been derived from high-resolution spectra via atomic data and line-blanketed model atmospheres. DY Cen is shown to be a metal-poor EHe star whose composition supports an anticorrelation be…

1993 Astronomy and Astrophysics
IUE 49
A Cluster of Nascent Galaxies at Z = 2?
DOI: 10.1086/186740 Bibcode: 1993ApJ...404L..45D

Dressler, Alan; Oemler, Augustus, Jr.; Gunn, James E. +1 more

On a 6 hr Wide Field Camera exposure with the Hubble Space Telescope of the rich cluster CL 0939+4713, we have identified an apparent cluster of ~30 faint, extended objects with magnitudes 22 < r < 25. The objects are typically 1" in size with bright central regions only a few tenths of an arcsecond in size, and are distributed over a region…

1993 The Astrophysical Journal
eHST 49
Excitation Rate Coefficients and Line Ratios for the Optical and Ultraviolet Transitions in S II
DOI: 10.1086/191824 Bibcode: 1993ApJS...88..329C

Cai, Wei; Pradhan, Anil K.

New calculations are reported for electron excitation collision strengths, rate coefficients, transition probabilities, and line ratios for the astrophysically important optical and UV lines in S II. The collision strengths are calculated in the close coupling approximation using the R-matrix method. The present calculations are more extensive tha…

1993 The Astrophysical Journal Supplement Series
IUE 48
UV spectral variability in the Herbig AE star HR 5999. 11: The accretion interpretation
Bibcode: 1993A&A...274..381P

Grady, C. A.; Perez, M. R.; The, P. S.

We report recent IUE high- and low-dispersion observations with the IUE long wavelength camera (LWP) and short wavelength camera (SWP) of the Herbig Ae star HR 5999. We have found a dramatic change in the structure of the Mg II h and k lines (2795.5, 2802.7 Å) along with some continuum flux excesses especially at the short end of the SWP camera. L…

1993 Astronomy and Astrophysics
IUE 47
Low-frequency electromagnetic plasma waves at comet P/Grigg-Skjellerup analysis and interpretation
DOI: 10.1029/93JA02532 Bibcode: 1993JGR....9820937N

Coates, A. J.; Neubauer, Fritz M.; Glassmeier, Karl-Heinz +1 more

The propagation and polarization characteristics of low-frequency electromagnetic wave fields near comet P/Grigg-Skjellerup (P/GS) are analyzed using magnetic field and plasma observations obtained by the Giotto magnetometer experiment and the Johnstone plasma analyzer during the encounter at the comet on July 10, 1992. The results have been physi…

1993 Journal of Geophysical Research
Giotto 47