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Ulysses measurements of energetic H3 molecules in Jupiter's magnetosphere
DOI: 10.1029/93JA02589 Bibcode: 1993JGR....9821145L

Lanzerotti, L. J.; Maclennan, C. G.; Feldman, D. M.

The Voyager 2 measurements of energetic (~1 MeV/nucleon) H3 molecules in Jupiter's magnetosphere provided strong evidence that the planet's ionosphere is an important plasma source in the Jovian environment (Hamilton et al., 1980). During the Ulysses spacecraft encounter with Jupiter in February 1992 the Heliosphere Instrument for Spect…

1993 Journal of Geophysical Research
Ulysses 8
Ulysses observations of the planetary depletion layer at Jupiter
DOI: 10.1016/0032-0633(93)90093-H Bibcode: 1993P&SS...41..857H

Smith, E. J.; Bame, S. J.; Phillips, J. L. +2 more

The repeated samplings of the Jovian magnetosheath during the Ulysses encounter with Jupiter provided an opportunity to probe the planetary depletion layer. Of the 10 complete crossings of the Jovian magnetopause, only three contained clear signatures of an overlying depletion layer. All of these occurred on the flanks of the magnetosphere near th…

1993 Planetary and Space Science
Ulysses 8
Radiative energy flux changes of PLEIONE in the far-UV through the Be-shell ---> Be transition.
Bibcode: 1993A&A...269..415D

Mauron, N.; Doazan, V.; Barylak, M. +2 more

We present far UV observations of Pleione made with the IUE satellite in the time-interval 1979-1991 which show, for the first time in the wavelength range 1250-3000 A, the dramatic changes of the FUV radiative energy flux between the Be-shell and the Be phases of a Be star. Between 1979, when Pleione exhibited a strong shell spectrum, and 1991, w…

1993 Astronomy and Astrophysics
IUE 8
Spectroscopic binary orbits from ultraviolet radial velocities. Paper 11: delta Circini (HD 135240)
Bibcode: 1993Obs...113..139S

Stickland, D. J.; Pachoulakis, I.; Koch, R. H. +1 more

1993 The Observatory
IUE 8
Spectrophotometric behavior of 56 Arietis.
Bibcode: 1993A&A...268..187S

Stepien, K.; Czechowski, W.

Archival IUE and published visual spectrophotometric data on the magnetic CP star 56 Ari are combined in nearly 20 energy distributions for different phases of the rotational cycle. Comparison with spectral variations shows that the light variations in the shortest wavelength region are strongly influenced by the nonuniformity of the silicon distr…

1993 Astronomy and Astrophysics
IUE 8
Far-Ultraviolet Stellar Photometry: A Field in Orion
DOI: 10.1086/191847 Bibcode: 1993ApJS...89..259S

Schmidt, Edward G.; Carruthers, George R.

Far-ultraviolet photometry for 625 objects in Orion is presented. These data were extracted from electrographic camera images obtained during sounding rocket flights in 1975 and 1982. The 1975 images were centered close to the belt of Orion while the 1982 images were centered approximately 9 deg further north. One hundred and fifty stars fell in t…

1993 The Astrophysical Journal Supplement Series
IUE 8
Diffusive Shock Acceleration and the November 1991 Event Particle Diffusion Mean Free Paths as Observed from 'ULYSSES'
Bibcode: 1993ICRC....3..270Q

Keppler, E.; Quenby, J. J.; Drolias, B. +2 more

1993 23rd International Cosmic Ray Conference (ICRC23), Volume 3
Ulysses 8
Hubble Space Telescope Observations of the Galactic Center Region at 1.02 Microns
DOI: 10.1086/116741 Bibcode: 1993AJ....106.1484L

Becklin, E. E.; Liu, T.; Henry, J. P. +1 more

We present HST observations of the galactic center region using the Planetary Camera with the F1042M filter at an effective wavelength of 1.02 micron. We detect several infrared sources seen at this wavelength before but with angular resolution better than previous observations. Our data reveal the source GZ A which was first seen by Rosa et al. (…

1993 The Astronomical Journal
eHST 7
Heavy mass loss from the symbiotic star AS 304.
DOI: 10.1093/mnras/263.1.267 Bibcode: 1993MNRAS.263..267M

Munari, Ulisse; Buson, Lucio M.

IUE, optical and infrared observations of the previously poorly studied symbiotic star AS 304 are discussed. The IUE low-resolution spectra are dominated by very strong P Cygni profiles of the resonant lines of N v, Si IV and C IV, indicating that the hot component of AS 304 is losing mass at a high rate via a fast wind. These P Cygni profiles mak…

1993 Monthly Notices of the Royal Astronomical Society
IUE 7
Composition of Interplanetary Ions in Recurrent Events: Measurements by HI-SCALE on Ulysses at 3-5 A.U.
Bibcode: 1993ICRC....3..330M

Tappin, S. J.; Lanzerotti, L. J.; Gold, R. E. +2 more

1993 23rd International Cosmic Ray Conference (ICRC23), Volume 3
Ulysses 7