Observational and theoretical studies of rich clusters with multiple subcondensations

Details Observational and theoretical studies of rich clusters with multiple subcondensations Observational and theoretical studies of rich clusters with multiple subcondensations

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sao..reptr....g&link_type=abstract

Semiannual Report, 1 Jan. - 30 Jun. 1984 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Cosmology, Galaxies, Red Shift, Star Distribution, Stellar Evolution, Velocity Distribution, Computerized Simulation, Data Bases, Statistical Analysis, Stellar Motions, Stellar Structure, Virgo Galactic Cluster

Scientific paper

Observational and theoretical studies of the formation and evolution of clusters of galaxies are investigated. The relationship between the properties of individual galaxies and their environment is examined. Perphaps the most remarkable physical result derived from these is the apparent substructure in redishift position space. The distribution of spiral galaxies is quite different from the distribution of the ellipticals. The velocity distribution for the spirals is also substantially broader than the distribution for the ellipticals.

Affiliated with

Also associated with

No associations

Rating

Observational and theoretical studies of rich clusters with multiple subcondensations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Observational and theoretical studies of rich clusters with multiple subcondensations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational and theoretical studies of rich clusters with multiple subcondensations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1856028