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The 1986FEB Solar Activity - a Comparison of Giotto VEGA-1 and IMP-8 Soalr Wind Measurements with Magnetohydrodynamic Simulations
DOI: 10.1007/BF00152293 Bibcode: 1991SoPh..132..353D

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

Large disturbances in the interplanetary medium were observed by several spacecraft during a period of enhanced solar activity in early February 1986. The locations of six solar flares and the spacecraft considered here encompassed more than 100° of heliolongitude. These flares during the minimum of cycle 21 set the stage for an extensive multi-sp…

1991 Solar Physics
Giotto 16
Photometric and spectroscopic studies of cool stars discovered in EXOSAT X-ray images. I. Time variability and spectral classification of eight southern stars.
Bibcode: 1991A&AS...87..233C

Tagliaferri, G.; Pasquini, L.; Pallavicini, R. +4 more

As part of a larger program to study the optical properties of serendipitous Exosat sources, optical photometry and low-resolution spectroscopy are presented for eight southern stars which have been identified as optical counterparts of Exosat sources. X-ray flux variability has been detected for three of them. In all three cases the optical count…

1991 Astronomy and Astrophysics Supplement Series
Exosat 16
The UV variability of the intermediate polars TW Pictoris (H 0534-581) and TX Columbae (1H 0542-407).
Bibcode: 1991A&A...250...99M

Bonnet-Bidaud, J. M.; Buckley, D. A. H.; Mouchet, M. +1 more

UV observations of two X-ray sources suggested to be nonsynchronous magnetic cataclysmic binaries (TW Pic and TX Col) are reported. Each source was observed at different epochs with simultaneous optical photometry in one case (TW Pic). The UV spectrum of both sources is typical of intermediate polars, showing a blue continuum with strong N V, C IV…

1991 Astronomy and Astrophysics
IUE 16
The SI II intercombination multiplet in late-type stars.
DOI: 10.1093/mnras/253.3.474 Bibcode: 1991MNRAS.253..474D

Dufton, P. L.; Keenan, F. P.; Byrne, P. B. +3 more

New atomic data are used to calculate the relative intensities of transitions within the Si II 3s(2)3p(2)P-3s3p(2) 4P intercombination multiplet for plasma parameters appropriate to late-type stellar atmospheres. These ratios are found to be significantly different from those of Dufton and Kingston, (1991), principally due to changes in the radiat…

1991 Monthly Notices of the Royal Astronomical Society
IUE 16
A Study of the Young Massive Cluster N90 in the SMC
DOI: 10.1086/115737 Bibcode: 1991AJ....101..933H

Thompson, I. B.; Hutchings, J. B.; Cartledge, S. +1 more

We present optical and UV spectra of O and B stars in the compact nebulous cluster Henize N90 in the SMC. The brightest stars are of type O and B, although our optical and UV classifications do not all agree closely. We discuss the spectra, effective temperatures, bolometric luminosities, extinction, stellar winds, and the evolutionary state of th…

1991 The Astronomical Journal
IUE 15
Quasi-periodic oscillations in short type II bursts from the Rapid Burster.
DOI: 10.1093/mnras/249.2.300 Bibcode: 1991MNRAS.249..300L

Stella, L.; van Paradijs, J.; van der Klis, M. +4 more

The authors present and discuss new information on quasi-periodic oscillations (QPO) in type II bursts from the Rapid Burster, which are under 30 sec in duration.

1991 Monthly Notices of the Royal Astronomical Society
Exosat 15
EXOSAT observations of the X-ray burst source 4U 1702-42.
Bibcode: 1991A&A...250..389O

van Paradijs, J.; van der Klis, M.; Lewin, W. H. G. +2 more

The two Exosat observations of 4U 1702 - 42 are reported. In one of them three bursts are detected. The bursts and the spectral and fast-temporal behavior of the persistent emission are analyzed. It is concluded that 4U 1702 - 42 is an atoll source, which was in the banana state when the bursts were present. The characteristics of the burst are si…

1991 Astronomy and Astrophysics
Exosat 15
The nature of the F STR lambda 4077 stars. IV. Search for white dwarfs around barium dwarfs.
Bibcode: 1991A&A...251..489N

Lanz, T.; North, P.

The energy distribution of three stars classified as F str 4077-A by Bidelman has been observed in the ultraviolet with the IUE satellite. Although the stars examined have the same kind of abundance anomalies as the Ba giants and Bond's CH subgiants (i.e. an overabundance of s-process elements), no UV excess related with the presence of the expect…

1991 Astronomy and Astrophysics
IUE 15
The Ultraviolet Spectrum of Scorpius X-1 as Observed by IUE: 1978--1988
DOI: 10.1086/169855 Bibcode: 1991ApJ...370..717K

Raymond, J. C.; Kallman, T. R.; Vrtilek, S. D.

The IUE observations of Sco X-1 taken prior to September 1988 are summarized. These data are tested for variability associated with orbital motion and for correlations between the various observables. The continuum spectra are fitted to simple models for accretion disk atmospheres which demonstrate that X-ray heating dominates the outer regions of…

1991 The Astrophysical Journal
IUE 15
Spectral transformation of the unusual variable star MWC560 to resemble a nova
DOI: 10.1038/350404a0 Bibcode: 1991Natur.350..404M

Sonneborn, George; Maran, Stephen P.; Oliversen, Ronald J. +1 more

MWC560 is an emission-line star catalogued1in 1943 and later described2 as an 'extraordinary symbiotic-like variable'. It was recently found3 to be undergoing a photometric and spectroscopic outburst. A dramatic change has occurred in the ultraviolet spec-trum of MWC560, so that it now closely resembles the spectru…

1991 Nature
IUE 15