Redshift observation of Shakhbazyan's compact groups of galaxies and their number-diameter relation

Details Redshift observation of Shakhbazyan's compact groups of galaxies and their number-diameter relation Redshift observation of Shakhbazyan's compact groups of galaxies and their number-diameter relation

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasj...43..169k&link_type=abstract

Astronomical Society of Japan, Publications (ISSN 0004-6264), vol. 43, no. 1, 1991, p. 169-176.

Other

15

Cosmology, Galactic Clusters, Red Shift, Density (Number/Volume), Spatial Distribution, Spectrographs

Scientific paper

The redshifts of four of Shakhbazyan's compact groups of galaxies (SCGG 253, 351, 352, and 357) were determined to be z = 0.073, 0.030, 0.049, and 0.076, respectively. The number-diameter relation of Shakhbazyan's compact groups was investigated based upon these redshift data, together with those obtained in previous studies for SCGG 202, 205, 223, 245, and 348, as well as those reported by other observers for SCGG 1, 4, and 123. The majority of SCGG's were found to approximately follow an empirical number-diameter relation.

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