Addendum: Why There Are No Elliptical Galaxies More Flattened Than E7. Thirty Years Later, Published in Serb. Astron. J. No. 173 (2006), 13-33

Details Addendum: Why There Are No Elliptical Galaxies More Flattened Than E7. Thirty Years Later, Published in Serb. Astron. J. No. 173 (2006), 13-33 Addendum: Why There Are No Elliptical Galaxies More Flattened Than E7. Thirty Years Later, Published in Serb. Astron. J. No. 173 (2006), 13-33

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007seraj.174...89c&link_type=abstract

Serbian Astronomical Journal, vol. 174, p. 89-90

Astronomy and Astrophysics

Astronomy

1

Cosmology: Dark Matter, Galaxies: Evolution, Galaxies: Formation, Galaxies: Haloes, Galaxies: Structure

Scientific paper

The existence of some sort of instability with regard to prolate configurations has been advocated in an earlier paper (Caimmi 2006) in order to explain the observed lack of elliptical galaxies more elongated than E7. It is recognized that a viable physical process might be the occurrence of bending instabilities, which were fully investigated long time ago, both analytically (Polyachenko and Shukhman 1979) and numerically (Merritt and Hernquist 1991).

Affiliated with

Also associated with

No associations

Rating

Addendum: Why There Are No Elliptical Galaxies More Flattened Than E7. Thirty Years Later, Published in Serb. Astron. J. No. 173 (2006), 13-33 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 Addendum: Why There Are No Elliptical Galaxies More Flattened Than E7. Thirty Years Later, Published in Serb. Astron. J. No. 173 (2006), 13-33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Addendum: Why There Are No Elliptical Galaxies More Flattened Than E7. Thirty Years Later, Published in Serb. Astron. J. No. 173 (2006), 13-33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1720767