Combined ultraviolet studies of astronomical sources

Details Combined ultraviolet studies of astronomical sources Combined ultraviolet studies of astronomical sources

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983sao..reptr....d&link_type=abstract

Semiannual Progress Report, 1 Feb. - 31 Jul. 1983 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astronomy

Astronomy, Shock Waves, Ultraviolet Radiation, F Stars, High Temperature Gases, Spectrophotometry

Scientific paper

Ultraviolet spectra of non-radiataive shock waves grain destruction and elemental abundances in interstellar shocks, carbon abundance in M33 and M31 from supernova remnants, determination of the mass function in the large Magellanic cloud, UV spectra of white dwarf pulsars, stellar flares, availability of the double quasar Q 0957 + 56' AB, spectra of late-F dwarfs and their relation to rotation, dynamics of hot gas surrounding hybrid stars, high resolution study of epsilon coronae Austriual, active regions on solar-type dwarfs as a function of rotation rate and age, coordinated chromospheric synoptic observations of selected late-type stars, the two-component atmosphere of Lambda Andromedae, and activity in Hyades giants are discussed.

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