SC 2059-247 - No evidence for cluster evolution or extreme X-ray properties

Details SC 2059-247 - No evidence for cluster evolution or extreme X-ray properties SC 2059-247 - No evidence for cluster evolution or extreme X-ray properties

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...192...77k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988, p. 77-80.

Astronomy and Astrophysics

Astronomy

1

Brightness Distribution, Galactic Clusters, Mass Flow, X Ray Astronomy, Bl Lacertae Objects, Exosat Satellite, Luminosity

Scientific paper

The southern cluster SC 2059-247 has been observed by the X-ray
satellite EXOSAT. The cluster has a high luminosity and cooling mass
flow and a small core radius, but it has neither exceptional properties
compared to other clusters, nor does it show signs of evolution effects,
as was concluded from earlier Einstein observations.

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