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A Catalog of X-Ray Spectra of BL Lacertae Objects
DOI: 10.1086/191755 Bibcode: 1993ApJS...85..111C

Bassani, L.; Ciliegi, P.; Caroli, E.

This paper contains a list of X-ray spectra of BL Lac objects mostly collected from the literature. For a small sample of objects EXOSAT/ME spectra have also been analyzed and included in this list. In the catalog 42 objects are considered (26 radio selected and 16 X-ray selected) for a total of 311 X-ray spectra. For each object we report the X-r…

1993 The Astrophysical Journal Supplement Series
Exosat 23
Ulysses observations of noncorotational flows in the outer dayside Jovian magnetosphere
DOI: 10.1016/0032-0633(93)90098-M Bibcode: 1993P&SS...41..931S

Balogh, A.; Forsyth, R. J.; Cowley, S. W. H. +3 more

Using data from the Anisotropy Telescopes on the Ulysses spacecraft obtained during the February 1992 encounter with Jupiter, we have derived the bulk velocity of ions in the energy range 0.7-1.3 MeV which were detected in Jupiter's outer magnetosphere (at a jovicentric distance of between ∼80 and ∼110 RJ). The derived ion bulk velocity…

1993 Planetary and Space Science
Ulysses 23
High-velocity tails on the velocity distribution of solar wind ions
DOI: 10.1029/92JA02902 Bibcode: 1993JGR....98.3605O

Geiss, J.; Gloeckler, G.; Wilken, B. +2 more

Recent observations of the solar wind using the SWICS instrument on the Ulysses spacecraft have shown the presence of high-velocity ``tails'' on the velocity distribution of protons. Similar features have also been observed on the velocity distributions of helium and oxygen ions. Of the order of 1% of the solar wind density is involved in these ta…

1993 Journal of Geophysical Research
Ulysses 23
Detection of [O ii] lambda 2471 from the Io Plasma Torus
DOI: 10.1086/187031 Bibcode: 1993ApJ...415L..55M

Feldman, P. D.; Moos, H. W.; Strobel, D. F. +2 more

We report the first detection of the O II 2471-A forbidden line from the Io plasma torus. Observations of the east and west torus ansae at 5.7 R(J) on 1992 March 15 and May 1, respectively, using the Goddard High Resolution Spectrograph of the HST have resulted in about 5-sigma detections of the line on both occasions, with line brightnesses of 30…

1993 The Astrophysical Journal
eHST 22
Short Communication: Optical probing of dust in comet Grigg-Skjellerup from the Giotto spacecraft
DOI: 10.1016/0032-0633(93)90046-5 Bibcode: 1993P&SS...41..167L

Bertaux, J. L.; Levasseur-Regourd, A. C.; Renard, J. B. +3 more

The optical probe experiment (OPE) has provided the first in situ high-resolution optical probing of the very inner coma of a short period comet, during the 10 July 1992 encounter of the Giotto spacecraft with Grigg-Skjellerup. Preliminary results of the encounter are presented below. Indications of entering the dust coma occurred around 17,000 km…

1993 Planetary and Space Science
Giotto 22
The Spectrum of the Central Star of the Planetary Nebula in M22
DOI: 10.1086/186923 Bibcode: 1993ApJ...411L.103H

Harrington, J. P.; Paltoglou, George

New optical observations of the central star of the planetary nebula IRAS 18333-2357 in the globular cluster M22 show lines of H I, He II, C IV, N IV, and N V. The spectrum closely resembles the sdO star KS 292, which has surface abundances enhanced by products of hydrogen shell burning and helium burning, and an effective temperature of 75,000 K.…

1993 The Astrophysical Journal
IUE 22
Optically thin H Lyman alpha production on outer planets: Low-energy proton acceleration in parallel electric fields and neutral H atom precipitation from ring current
DOI: 10.1029/92JA02400 Bibcode: 1993JGR....98.9473B

Bhardwaj, A.; Singhal, R. P.

A Monte Carlo model has been constructed to describe the energization and energy degradation of low-energy protons in an H2 atmosphere in the presence of parallel electric field. The energy spectrum of Ly α collision events is employed to determine the volume emission rate (VER) of H Ly α emissions. Numerical experiments have been perfo…

1993 Journal of Geophysical Research
IUE 22
Intergalactic and galactic clouds on the line of sight to SN 1993J in M 81 seen in IUE spectra.
Bibcode: 1993A&A...280L..15D

Bomans, D. J.; Fransson, C.; Kirshner, R. P. +4 more

High resolution IUE spectra of SN 1993J in M81 show the existence of several clouds on the line of sight. These include local galactic gas at 0 km s^-1^, gas in M81 at -130 km s^-1^, a cloud in the halo of the Milky Way near -45 km s^-1^, and an intergalactic cloud near +140 km s^-1^. Arguments for each of these locations are given. There is littl…

1993 Astronomy and Astrophysics
IUE 22
Mass loading and velocity diffusion models for heavy pickup ions at comet Grigg-Skjellerup
DOI: 10.1029/93JA02531 Bibcode: 1993JGR....9820995H

Coates, A. J.; Neubauer, Fritz M.; Johnstone, A. D. +1 more

We compare model predictions of cometary water group ion densities and the solar wind slow down with measurements made by the Giotto Johnstone plasma analyzer implanted ion sensor at the encounter with comet Grigg-Skjellerup (G-S) on July 10, 1992. The observed slope of the ion density profile on approach to the comet is unexpectedly steep. Possib…

1993 Journal of Geophysical Research
Giotto 22
Core sub-structure of elliptical galaxies : the core resolution technique applied to NGC 1399.
Bibcode: 1993A&A...277..421S

Stiavelli, M.; Zeilinger, W. W.; Moller, P.

UBRJK' images, obtained with subarcsecond seeing, are presented and used to derive the core light profile of the elliptical galaxy NGC 1399. These data, combined with an HST PC V band exposure, and high- resolution velocity dispersion data obtained by us are used to show that NGC 1399 is likely to possess a central dark mass concentration. Models …

1993 Astronomy and Astrophysics
eHST 22