Galactic halos, globular clusters and massive neutrinos

Details Galactic halos, globular clusters and massive neutrinos Galactic halos, globular clusters and massive neutrinos

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..82..249f&link_type=abstract

Astrophysics and Space Science, vol. 82, no. 1, Feb. 1982, p. 249-253.

Astronomy and Astrophysics

Astrophysics

6

Cosmology, Galactic Evolution, Globular Clusters, Halos, Neutrinos, Red Shift, Baryons, Gravitational Effects, Mass Distribution, Microwaves, Photons

Scientific paper

Within the framework of a Gamow cosmology with massive neutrinos, a situation is envisioned in which both galactic halos and globular clusters form as a result of the existence of a 'critical injection mass'. Here, globular clusters are formed primordially (z equal to about 1,000), and only later (z approximately 10-100) are then clustered into galaxies by the gravitational instability of neutrinos. Some of the globular clusters and uncondensed debris form the galactic disks near the centers of the potential wells; other clusters remain in the neutrino halo. This explains why globular clusters are detected at several tens of kiloparsecs from disks of visible matter. Analysis of their motion can furnish additional information on the distribution of mass in the neutrino halos.

Affiliated with

Also associated with

No associations

Rating

Galactic halos, globular clusters and massive neutrinos 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 Galactic halos, globular clusters and massive neutrinos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Galactic halos, globular clusters and massive neutrinos will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1646652