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Echoes from an irradiated disc in GRO J1655-40
DOI: 10.1046/j.1365-8711.1998.01856.x Bibcode: 1998MNRAS.299L..37H

Horne, Keith; O'Brien, K.; Chen, W. +2 more

We demonstrate correlated rapid variability between the optical/UV and X-ray emission for the first time in a soft X-ray transient, GRO J1655-40: Hubble Space Telescope (HST) light curves show similar features to those seen by the Rossi X-ray Timing Explorer (RXTE), but with mean delay of up to 10-20s. We interpret the correlations as the result o…

1998 Monthly Notices of the Royal Astronomical Society
eHST 43
Power-Law Decays in the Optical Counterparts of GRB 970228 and GRB 970508
DOI: 10.1086/311403 Bibcode: 1998ApJ...500L.105G

Kouveliotou, C.; van Paradijs, J.; McClintock, J. E. +7 more

We report on RC- and K-band observations of the optical counterpart to GRB 970508 with the Fred Lawrence Whipple Observatory (FLWO) 1.2 m telescope. Eleven RC-band observations were obtained on 1997 May 12, and three on May 14. The counterpart clearly faded between the two nights. On May 12 there was no evidence for variabili…

1998 The Astrophysical Journal
eHST 43
Origin and production of C(^1D) atoms in cometary comae
Bibcode: 1998A&A...330..753T

Feldman, P. D.; Festou, M. C.; Tozzi, G. P.

The abundance of carbon atoms in the metastable (1) D state near the cometary nucleus provides an important diagnostic of one of the principal sources of carbon in the cometary coma. This quantity may be determined in two independent ways: measurement of (1) D -(1) P fluorescence at 1931 Angstroms and by prompt emission of the (1) D -(3) P doublet…

1998 Astronomy and Astrophysics
IUE 43
New study of the quasi-molecular Lyman alpha satellites due to H-H and H-H(+) collisions
Bibcode: 1998A&A...335.1124A

Gerbaldi, M.; Allard, N. F.; Kielkopf, J. +2 more

We present new theoretical calculations of the total profile of the atomic hydrogen Lyman alpha spectral line perturbed by collisions with neutral hydrogen atoms and protons. The variation of the radiative dipole moment during the collision is taken into account. This leads to an increase in the amplitude of the main spectral line satellites and t…

1998 Astronomy and Astrophysics
IUE 43
Long-term variability of the Be/X-ray binary A0535+26 - I. Optical and UV spectroscopy
DOI: 10.1046/j.1365-8711.1998.01257.x Bibcode: 1998MNRAS.294..165C

Coe, M. J.; Steele, I. A.; Buckley, D. A. H. +11 more

The results of a 7-yr optical and UV spectroscopic study of the high-mass X-ray binary A0535+26 are presented. It was found that throughout the period of the observations the line profile of Hα showed considerable variability. A correlation between the equivalent width of Hα and both V-band magnitude and (B-V) colour excess was observed, albeit wi…

1998 Monthly Notices of the Royal Astronomical Society
IUE 42
Cosmic-Ray Transport Coefficients
Bibcode: 1998SSRv...83..351G

Giacalone, Joe

A review of cosmic-ray transport coefficients, based on historic and recent observations and theoretical insights, is presented. Particular emphasis is on the transport of cosmic rays across the magnetic field, which is of foremost importance, and is presently poorly understood and widely debated.

1998 Space Science Reviews
Ulysses 42
Detection of Far-Infrared Water Vapor, Hydroxyl, and Carbon Monoxide Emissions from the Supernova Remnant 3C 391
DOI: 10.1086/311672 Bibcode: 1998ApJ...507L..93R

Reach, William T.; Rho, Jeonghee

We report the detection of shock-excited far-infrared emission of H2O, OH, and CO from the supernova remnant 3C 391, using the Infrared Space Observatory Long-Wavelength Spectrometer. This is the first detection of thermal H2O and OH emission from a supernova remnant. For two other remnants, W28 and W44, CO emission was detec…

1998 The Astrophysical Journal
ISO 42
The Lensing Cluster MS 0440+0204 Seen by HST, ROSAT, and ASCA. I. Cluster Properties
DOI: 10.1086/305471 Bibcode: 1998ApJ...497..573G

Le Fèvre, O.; Hammer, F.; Falco, E. E. +3 more

We present an analysis of the properties of the lensing cluster MS 0440+0204 at z = 0.1965. MS 0440+0204 has been observed with a variety of telescopes at diverse wavelengths: from the ground with the Canada-France-Hawaii Telescope, the Multiple Mirror Telescope, and the Keck Telescope, and from the Earth orbit with HST, ROSAT, and ASCA. Mass dete…

1998 The Astrophysical Journal
eHST 42
Energetic (∼ 1 to 50 MeV) protons associated with Earth-directed coronal mass ejections
DOI: 10.1029/98GL50062 Bibcode: 1998GeoRL..25.2525T

Laitinen, T.; Vainio, R.; Valtonen, E. +7 more

During the period from January through mid-May, 1997, four large Earth-directed CMEs were observed by the Large Angle Spectroscopic Coronograph (LASCO). These CMEs were associated with long-lasting fluxes of >1.6 MeV protons detected by the Energetic and Relativistic Nuclei and Electron instrument (ERNE). However, the magnitudes of energetic pr…

1998 Geophysical Research Letters
SOHO 42
Evidence for low-level AGN activity in the nucleus of the LINER galaxy NGC4594
DOI: 10.1046/j.1365-8711.1998.01944.x Bibcode: 1998MNRAS.300..893N

Filippenko, A. V.; Ho, L. C.; Reichert, G. A. +4 more

We investigate the properties of the low-ionization nuclear emission-line region (LINER) galaxy, NGC4594, using data taken with the Faint Object Spectrograph on the Hubble Space Telescope (HST) and with the ASCA X-ray observatory. The ultraviolet spectrum shows only narrow-line emission (FWHM ~800-1000 km s^-1) with no evidence for broad emission-…

1998 Monthly Notices of the Royal Astronomical Society
eHST 42