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Observational Properties of the Shakhbazian Groups SHKH 30 and SHKH 360

Published online by Cambridge University Press:  26 July 2016

H. Tiersch ,
H. Oleak ,
D. Stoll  and
H. Böhringer
H. Tiersch
Affiliation:
WIP-Gruppe “Astronomie” bei der Universität Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
H. Oleak
Affiliation:
WIP-Gruppe “Astronomie” bei der Universität Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
D. Stoll
Affiliation:
WIP-Gruppe “Astronomie” bei der Universität Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
H. Böhringer
Affiliation:
MPI Extraterrestrische Physik, D-85740 Garching, Germany

Extract

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X-ray emission has been detected from 12 compact groups of galaxies of the Shakhbazian catalogue (out of 27 investigated groups) with the ROSAT PSPC all-sky survey. The groups Shkh 30 (Shakhbazian 1973) and Shkh 360 (Petrosian 1978) are presented here (Figs. 1 and 2).

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 623 - 625
Copyright
Copyright © Kluwer 1994 

References

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Tiersch, H., Stoll, D., Oleak, H. and Böhringer, H., 1993a. ‘Observational properties of Shakhbazian groups’. Poster presented at the Spring Meeting of the Astronomische Gesellschaft, Kiel, March 8–12, 1993.Google Scholar
Tiersch, H. Stoll, D., Oleak, H., Böhringer, H. and MacGillivray, H.T., 1993b. ‘Optical and X-ray data of some Shakhbazian galaxy groups’. Poster presented at the 2nd General Meeting of the European Astronomical Society, Torun, August 18–21, 1993.Google Scholar