Studies of X-ray clusters of galaxies/intergalactic plasmas

Details Studies of X-ray clusters of galaxies/intergalactic plasmas Studies of X-ray clusters of galaxies/intergalactic plasmas

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984uat..reptq....s&link_type=abstract

Final Report Arizona Univ., Tucson.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Emission, Galaxies, Interstellar Space, Space Plasmas, Spectrographs, X Rays, Clouds, Data Reduction, Interstellar Gas, Line Spectra, Radial Velocity, Seyfert Galaxies, Spectral Resolution

Scientific paper

Intergalactic plasmas were investigated from both an observational and theoretical point of view. A multiobject spectrometer, the MX spectrograph was used to obtain detailed dynamical information on clusters of galaxies; this information was then compared with X ray emission from hot gas in these clusters. Several spectra of galaxies are presented, and data reduction of the spectra was discussed. The existence of quasar winds in Seyfert galaxies and the interaction between such a wind and the interstellar medium also were considered.

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