Search Publications

Reappearance of recurrent low-energy particle events at Ulysses/HI-SCALE in the northern heliosphere
DOI: 10.1029/97JA00640 Bibcode: 1997JGR...10211251R

Simnett, G. M.; Lanzerotti, L. J.; Armstrong, T. P. +4 more

In the high-latitude northern hemisphere of the heliosphere, the Heliosphere Instrument for Spectra Composition and Anisotropy at Low Energies (HI-SCALE) energetic particle detectors on Ulysses have measured quasi-recurrent ~26-day increases of 40-65 keV electrons during 11 solar rotations from October 1995 through July 1996. They do not appear on…

1997 Journal of Geophysical Research
Ulysses 23
Abundance analysis of the slow nova PW Vulpeculae 1984
DOI: 10.1093/mnras/290.1.75 Bibcode: 1997MNRAS.290...75S

Shore, Steven N.; Hauschildt, Peter H.; Schwarz, Greg J. +1 more

We determine the elemental abundances for the ejecta of the slow nova PW Vul 1984. Our technique uses a minimization of the emission-line fits of a photoionization model to available ultraviolet, optical and infrared spectra. We find the following abundances (by number) with respect to solar: He/H=1.0+/-0.4, C/H=7.0^+7_-4, N/H=85^+59_-41 and O/H=6…

1997 Monthly Notices of the Royal Astronomical Society
IUE 23
Evidence for an Anomalous State in the Black Hole Candidate 4U 1630-47
DOI: 10.1086/310413 Bibcode: 1997ApJ...474L..47K

Kuulkers, Erik; van der Klis, Michiel; Parmar, Arvind N.

We have reanalyzed two EXOSAT medium-energy observations during part of the 1984 X-ray outburst of the black hole candidate transient system 4U 1630-47. One observation (May 10) shows fast-timing properties (on timescales shorter than ~250 s) typical of those of other black hole candidates in their high states. The power spectrum shows a power law…

1997 The Astrophysical Journal
Exosat 22
Gamma-Ray Burst Arrival Time Localizations: Simultaneous Observations by Mars Observer, Compton Gamma Ray Observatory, and ULYSSES
DOI: 10.1086/312993 Bibcode: 1997ApJS..110..157L

Hurley, K. C.; Fishman, G. J.; Kouveliotou, C. +12 more

Between 1992 October 4 and 1993 August 1, concurrent coverage by the Compton Gamma Ray Observatory (CGRO), Mars Observer (MO), and Ulysses spacecraft was obtained for 78 gamma-ray bursts (GRBs). Although most of these were below the MO and Ulysses thresholds, nine were positively detected by all three spacecraft, with data quality adequate for qua…

1997 The Astrophysical Journal Supplement Series
Ulysses 22
Dynamic Processes in Be Star Atmospheres. VI. Simultaneous X-Ray, Ultraviolet, and Optical Variations in λ Eridani
DOI: 10.1086/304045 Bibcode: 1997ApJ...481..479S

Smith, Myron A.; Corcoran, M. F.; Murakami, T. +4 more

We document the results of simultaneous wavelength monitoring of the B2e star λ Eri. This campaign was carried out from ground stations and with the ROSAT, ASCA, IUE, and Voyager 2 space platforms during a week in 1995 February-March a smaller follow-up was conducted in 1995 September. During the first of these intervals λ Eri exhibited extraordin…

1997 The Astrophysical Journal
IUE 22
HST synthetic spectral analysis of U GEM in early and late quiescence: A heated white dwarf and accretion belt?
DOI: 10.1086/118547 Bibcode: 1997AJ....114.1165C

Horne, Keith; Sion, E. M.; Huang, M. +3 more

We have re-examined two archival HST FOS G130H spectra of the prototype dwarf nova U Geminorum obtained during its quiescence 13 days and 70 days after a wide outburst. Using synthetic spectral fitting with two flux-emitting components, a slowly rotating white dwarf photosphere, and a rapidly spinning accretion belt (Vrot sin i=3200 km …

1997 The Astronomical Journal
eHST 22
Near Infrared Imaging of the Hubble Deep Field with the Keck Telescope
DOI: 10.1086/118269 Bibcode: 1997AJ....113..474H

Hogg, David W.; Matthews, K.; Soifer, B. T. +4 more

Two deep K-band (2.2 microns ) images, with point-source detection limits of K=25.2 mag (one sigma), taken with the Keck Telescope in subfields of the Hubble Deep Field, are presented and analyzed. A sample of objects to K=24 mag is constructed and V606-I814 and I814-K colors are measured. By stacking visually sele…

1997 The Astronomical Journal
eHST 22
The Nuclear Region of M51 Imaged with the HST Planetary Camera
DOI: 10.1086/118246 Bibcode: 1997AJ....113..225G

Lauer, Tod R.; Faber, S. M.; Grillmair, Carl J. +4 more

We present high-resolution, broad- and narrow-band, pre-refurbishment images of the central region of M51 taken with the Planetary Camera of the Hubble Space Telescope. The V-band images show a rather chaotic distribution of dust lanes, though some are oriented radially, roughly aligned with the major axis of the bar, and may be transporting gas t…

1997 The Astronomical Journal
eHST 22
Chromospheric Emission in Metal-poor Solar-Type Stars
DOI: 10.1086/310607 Bibcode: 1997ApJ...480L..47P

Schrijver, Carolus J.; Peterson, Ruth C.

Cool stars like the Sun show chromospheric activity, which is largely attributed to nonradiative sources of energy linked to rotationally driven magnetic fields. However, a nonmagnetic process, such as dissipation of acoustic waves, may operate side by side with the first process. We report detections of chromospheric emission reversals in Mg II 2…

1997 The Astrophysical Journal
eHST 22
The heliospheric modulation of galactic cosmic rays at solar minimum
DOI: 10.1016/S0273-1177(97)00297-4 Bibcode: 1997AdSpR..19..883P

Potgieter, M. S.

The observations acquired by the Ulysses spacecraft since launch, but especially during the recent fast latitude scan, have provided a comprehensive, 3-dimensional view of the inner heliosphere. Together with the observations by IMP 8, Pioneer 10 and the two Voyagers, a wealth of new observations on particles and fields enables us to improve signi…

1997 Advances in Space Research
Ulysses 22