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Interstellar C IV and SI IV in the Direction of Loop I
Freire Ferrero, R.
Nearby late-B and early-A stars show clear IS absorptions in Mg II, C II and other lines (IUE spectra). Some of them, in the Sco Cen direction, also show absorption features at C IV and Si IV line wavelengths. We discuss the possible formation of these lines in an intermediate temperature gas region between the dense and cold H I wall and the hot …
Evolution and Mass Loss of AGB Stars in the Small Magellanic Cloud
Waters, L. B. F. M.; Blommaert, J. A. D. L.; van Loon, J. Th. +7 more
Clues to the Evolution of Massive Stars from their Far-Infrared Environments
Marston, A. P.
The turbulent state of cometary ion pickup generated fluctuations near comet P/Halley
Krauklis, I.; Johnstone, A. D.
One of the principal effects of an outgassing comet is to introduce additional mass into the solar wind flow. This mass-loading process results in the generation of Alfvén waves via ion-cyclotron resonance. In the case of the Halley encounter this source of ``new'' fluctuations was introduced into a low speed solar wind 0.89 AU from the sun. Previ…
ISO-SWS Spectral Characterization of Stars
Heras, A. M.; Shipman, R. F.; Price, S. D. +6 more
Hst/uv Periodic Variations in the Intermediate Polar FO AQR
Mukai, K.; de Martino, D.; Buckley, D. A. H. +3 more
A preliminary analysis of high temporal HST UV spectroscopy, as well as SAAO BVRI photometry, has revealed that FO Aqr, differently from all previous observations, has changed from a spin dominated to an orbital dominated variability, both in lines and continuum. The spectral dependence of the orbital continuum, however, has not changed with time.…
ULYSSES Laps Sun, Inspires New Missions
Hellemans, Alexander
ISOPHOT Observations of VEGA and Vega-like Stars
Walker, H. J.; Heinrichsen, I.
Detailed ISOPHOT observations of the far infrared excess of α Lyrae (Vega) are presented. The data comprise photometry in the range 25µm to 200µm and high resolution 60µm scan data to compare with 60µm and 90µm oversampled maps. The dust disk around Vega is clearly resolved. In addition similar maps of HD98800, SAO226057, SAO186777 and α Piscis Au…
Acceleration in energetics ions (~1MeV) in corotating interaction regions
Balogh, A.; Forsyth, R. J.; Goldstein, B. E. +4 more
We have correlated the ~1 MeV proton intensity (J) measured at corotating reverse shocks detected by Ulysses near the ecliptic plane and in the southern hemisphere with the shock strength and shock normal angle. We find that J is essentially independent of the shock strength below 29 degS, whereas between 29 deg and 41 degS J showed a good correla…
Molecular Features in ISO-SWS Spectra of O-Rich Long-Period Variables
Hron, J.; Kerschbaum, F.; Aringer, B. +1 more