Search Publications

Crowded Field Photometry of M15 Using the TRIFFID Camera
Bibcode: 1996IrAJ...23...37B

Butler, R. F.; Redfern, R. M.; Shearer, J. A. L.

High-resolution imaging has been performed for a number of years using TRIFFID, the UCG/DIAS High Resolution Camera. Post-exposure image sharpening (PEIS) of TRIFFID data routinely produces resolution improvements up to the theoretical maximum factor of two. HST resolution remains superior but unlike TRIFFID it cannot be used for extended observat…

1996 Irish Astronomical Journal
eHST 1
Cosmic rays in the heliosphere.
DOI: 10.1007/BF02506668 Bibcode: 1996NCimC..19..777B

Bieber, J. W.

This rapporteur paper covers topics of anomalous cosmic rays, shock acceleration, modulation and transport theory, cosmic-ray gradients, corotating interaction regions, coronal-mass ejections, and solar neutrinos. Among the highlights are: conclusive proof that most anomalous cosmic rays are singly charged, undisputed detection of anomalous cosmic…

1996 Nuovo Cimento C Geophysics Space Physics C
Ulysses 1
Sir Robert Wilson, C.B.E., FRS
DOI: 10.1007/BF02424423 Bibcode: 1996Ap&SS.237....3W

Willis, Allan J.; Hartquist, Thomas W.

1996 Astrophysics and Space Science
IUE 1
A model for the accretion disk in the dwarf nova AB Draconis
DOI: 10.1016/0275-1062(96)00026-4 Bibcode: 1996ChA&A..20..183L

Li, Zong-yun; Zhu, Ci-sheng; Ding, Yue-rong

A least squares fit to the dwarf nova AB Dra shows that the continuum spectrum predicted by a blackbody accretion disk model can roughly account for the IUE observations during the time of the explosion, while small discrepancies can be attributed to recombination radiation of an optically thin atmosphere and/or blackbody radiation from hot spots.…

1996 Chinese Astronomy and Astrophysics
IUE 0
The Sun slowly gives up its secrets.
Bibcode: 1996AsNow..10...40P

Phillips, K.

A new understanding of the Sun is emerging from the Ulysses and Yohkoh probes.

1996 Astronomy Now
Ulysses 0
HIPPARCOS - ein Astrometrie-Satellit der ESA.
Bibcode: 1996A&R....33....4B

Bastian, U.

Die bisherigen Meßdaten des HIPPARCOS lassen sensationelle Ergebnisse erwarten.

1996 Astronomie und Raumfahrt
Hipparcos 0
Interplanetary magnetic field control of heavy ion abundances at ~ 5.2 AU
DOI: 10.1016/0273-1177(95)00590-B Bibcode: 1996AdSpR..17d.307L

Forsyth, R. J.; Lanzerotti, L. J.; Maclennan, C. G.

The HI-SCALE instrument on the Ulysses spacecraft measured a long-lasting heavy ion particle event from about day 304 to day 318, 1992, at a southern heliographic latitude of ~20 deg. An analysis is presented of the relative (to O) C and Fe abundance variations during this interval. The variations are associated with major interplanetary magnetic …

1996 Advances in Space Research
Ulysses 0
The mass and angular momentum loss from the edge of the accretion disc and the evolution of cataclysmic binaries.
Bibcode: 1996AcApS..16...41H

Yu, K. N.; Huang, Runqian

The IUE observations of high excitation P Cygni profiles provide evidence that there is mass outflow in the cataclysmic variables with speed of ≡5000 km/s which can not be driven by the late-type secondary stars. The authors proposed here that these outflows are originated from the outer edge of the accretion disc and give a model for calculation …

1996 Acta Astrophysica Sinica
IUE 0
Relative astrometry with Hipparcos: double stars with orbital motion.
Bibcode: 1996A&A...312.1038E

Badiali, M.; Cardini, D.; Emanuele, A. +2 more

During the Hipparcos data analysis an algorithm was developed to study orbital motion in double stars and to derive the seven Dommanget parameters in the positive cases. Three approaches were followed: linear motion model, quadratic motion model and orbital model. In the last model the algorithm needs sufficiently good starting values and it has b…

1996 Astronomy and Astrophysics
Hipparcos 0
Analyses of Wolf-Rayet ultraviolet spectra
DOI: 10.1007/BF00645495 Bibcode: 1996Ap&SS.238...71R

Rochowicz, Krzysztof

Ultraviolet spectra of population I WR stars obtained from IUE archive are used to determine fundamental stellar parameters. Terminal velocities for 85 galactic and LMC Wolf-Rayet stars were obtained by means of the empirical relation between spectral quantities easily measured in low resolution and high-resolution terminal velocity measurements. …

1996 Astrophysics and Space Science
IUE 0