Combined ultraviolet studies of astronomical source

Details Combined ultraviolet studies of astronomical source Combined ultraviolet studies of astronomical source

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985sao..reptr....d&link_type=abstract

Semiannual Progress Report, 1 Feb. - 31 Jul. 1985 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astronomy

Binary Stars, Cataclysmic Variables, Chromosphere, Cygnus Constellation, Dwarf Novae, Dwarf Stars, Giant Stars, Hercules Nova, Late Stars, Magellanic Clouds, Metallicity, Oxygen Spectra, Photoionization, Stellar Winds, Supernova Remnants, Ultraviolet Astronomy, X Ray Astronomy, Interstellar Gas, Photometry, Spectral Methods, Spectroscopy, Stellar Structure

Scientific paper

As part of its Ultraviolet Studies of Astronomical Sources the Smithsonian Astrophysical Observatory for the period 1 Feb. 1985 to 31 July 1985 observed the following: the Cygnus Loop; oxygen-rich supernova remnants in 1E0102-72; the Large Magellanic Cloud supernova remnants; P Cygni profiles in dwarf novae; soft X-ray photoionization of interstellar gas; spectral variations in AM Her stars; the mass of Feige 24; atmospheric inhomogeneities in Lambda Andromedae and FF Aquarii; photometric and spectroscopic observation of Capella; Alpha Orionis; metal deficient giant stars; M 67 giants; high-velocity winds from giant stars; accretion disk parameters in cataclysmic variables; chromospheric emission of late-type dwarfs in visual binaries; chromospheres and transient regions of stars in the Ursa Major group; and low-metallicity blue galaxies.

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