Studies of gas in cooling flow clusters

Details Studies of gas in cooling flow clusters Studies of gas in cooling flow clusters

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991huha.rept.....h&link_type=abstract

Final Report, 1 Nov. 1989 - 31 Oct. 1991 Hawaii Univ., Honolulu. Inst. for Astronomy.

Astronomy and Astrophysics

Astrophysics

Cooling Flows (Astrophysics), Emission Spectra, Galactic Clusters, Light Emission, Line Spectra, Stellar Coronas, X Ray Sources, X Ray Spectra, Astronomical Spectroscopy, Cosmic Dust, Infrared Astronomy Satellite, Interstellar Extinction, Iue, Satellite Observation

Scientific paper

This report describes studies of cooling flows in rich clusters of galaxies, found to be sources of strong, extended X-ray emission seen by the EINSTEIN satellite. Two complementary lines of investigation were pursued: (1) studies of the dust content of the cluster gas using multi-wavelength data from archival records of the IUE and IRAS satellites in combination with previously obtained optical, and (2) coronal line spectroscopic studies of the bright emission systems.

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