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The UV spectrum of the possible radio star HD 26676.
Stickland, D. J.
Results are reported for low-resolution UV spectroscopy (1150-1950 A and 1850-3250 A) of the star HD 26676, which may be associated with a weak nonthermal radio source, from the IUE satellite. It is found that the energy distribution of this star appears to be that of a perfectly normal single B8 V star. It is concluded that HD 26676 is an unlikel…
Heating of Chromospheres and Coronae in Cool Stars
Mullan, D. J.
Recent evidence is summarized that suggests that neither of two traditional views of chromospheric heating (that the flux of energy required to heat the solar chromosphere) is only a small fraction of the total radiative energy emerging from the solar interior and that chromospheres are heated by acoustic waves generated in the convection zone (wh…
I.U.E. observation of the CO molecule towards PSI Per (B5 Ve) and its implication.
Krishna Swamy, K. S.; Tarafdar, S. P.
International Ultraviolet Explorer probes the universe.
Hartline, B. K.
The impact of the International Ultraviolet Explorer (IUE), launched in January 1978, on ultraviolet astronomy is reviewed. An assortment of firsts has been achieved, including the first UV observation of a supernova, the first high-resolution UV spectrum of a star in another galaxy, and the first evidence that acetylene is present in the upper at…
International Ultraviolet Explorer Probes the Universe
Karplus Hartline, Beverly
IUE Observatory, European Space Agency, Villafranca Satellite Tracking Station. Report for the year 1978 January 1 to December 31.
Penston, M. V.; Macchetto, F.
IUE Observations of Circumstellar Lines and Mass Loss from a B-Star
Tarafdar, S. P.; Vardya, M. S.; Krishna-Swamy, K. S.
IUE observations of the planetary nebula NGC 7662.
Harrington, J. P.; Lutz, J. H.; Seaton, M. J.
Douze mois d'observation à l'aide du télescope orbitant « International Ultraviolet Explorer »
Houziaux, L.
The development and results of the first year of operation of the IUE astronomical satellite are outlined. The concept of the satellite is traced from the first proposal of the Large Astronomical Satellite by the precursor of ESA, through the proposed Ultraviolet Astronomical Satellite, the joint construction of the International Ultraviolet Explo…
Ariel 5 Hard X-Ray Observations
Coe, M. J.; Quenby, J. J.; Engel, A. R.
Results from the hard X-ray detector (8 cm2 area, 8 degrees f.w.h.m. field of view, energy range 26-1200 keV) are reviewed in the context of observations by other groups. At least three different classes of galactic sources are studied by this detector. In the first, magnetospheric control of the emission, which seems to be a modified t…