Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvl..57.2326z&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 57, Nov. 3, 1986, p. 2326-2329.
Astronomy and Astrophysics
Astrophysics
14
Galactic Evolution, Galactic Rotation, Space Density, Spiral Galaxies, String Theory, Density Distribution, Gravitational Collapse, Halos, Missing Mass (Astrophysics)
Scientific paper
Galactic halos seeded by loops of string in a universe dominated by dark matter fall into two categories: (1) Non-self-intersecting loops precipitate nearly spherically symmetric collapse and lead to a halo with low angular momentum J and a density profile ρ ≡ r-9/4. (2) Progeny of a self-intersecting primary loop recollapse into a single object which acquires J through tidal interactions. Its density profile, ρ ≡ r-2, is consistent with "flat rotation profiles" observed in spiral galaxies. It is tempting to identify these two types of string-seeded objects with (1) elliptical and (2) spiral galaxies.
No associations
LandOfFree
String-seeded spirals - Origin of rotation and the density of the halo 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 String-seeded spirals - Origin of rotation and the density of the halo, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and String-seeded spirals - Origin of rotation and the density of the halo will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1151162