Estimating the Mass Distribution of Galaxy Clusters from Observed Oblateness Ratios and Orientation of Background Galaxies

Details Estimating the Mass Distribution of Galaxy Clusters from Observed Oblateness Ratios and Orientation of Background Galaxies Estimating the Mass Distribution of Galaxy Clusters from Observed Oblateness Ratios and Orientation of Background Galaxies

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..932s&link_type=references

Astronomicheskii Zhurnal, Vol.70:5, P. 932, 1993

Astronomy and Astrophysics

Astronomy

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