Numerical model of the giant arc in Abell 963: an estimation of the deflector mass

Details Numerical model of the giant arc in Abell 963: an estimation of the deflector mass Numerical model of the giant arc in Abell 963: an estimation of the deflector mass

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992daec.conf...90a&link_type=abstract

In Distribution of Matter in the Universe, 2nd DAEC mtg, ed. G.A. Mamon and D. Gerbal (Meudon: Obs. de Paris) p. 90-93

Physics

Scientific paper

We have modeled giant luminous arcs (Fig. 1) found by Lavery and Henry
(1988) in the cluster Abell 963 (Fig. 2). There is, at least, three
times more lensing mass associated to the cluster than to the galaxies.
The source is probably a very faint galaxy (L <= 0.1 L*) which may be
a small spiral at z=0.77.

Affiliated with

Also associated with

No associations

Rating

Numerical model of the giant arc in Abell 963: an estimation of the deflector mass 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 Numerical model of the giant arc in Abell 963: an estimation of the deflector mass, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical model of the giant arc in Abell 963: an estimation of the deflector mass will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1114115