A combined X-ray and optical analysis of the galaxy cluster A2670

Details A combined X-ray and optical analysis of the galaxy cluster A2670 A combined X-ray and optical analysis of the galaxy cluster A2670

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.289..685h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 289, Issue 3, pp. 685-692.

Astronomy and Astrophysics

Astronomy

12

Galaxies: Clusters: General, Galaxies: Clusters: Individual: A2670, Cosmology: Observations, Large-Scale Structure Of Universe, X-Rays: General

Scientific paper

We analyse 15 ks of low-noise ROSAT PSPC data and calculate the mass distribution in A2670. The mass inferred from the X-ray data is not enough to explain the observed line-of-sight velocity dispersion profile, and we investigate two possible reasons for this. We conclude that A2670 is in the process of merging along the line of sight, as was first proposed by Bird.

Affiliated with

Also associated with

No associations

Rating

A combined X-ray and optical analysis of the galaxy cluster A2670 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 A combined X-ray and optical analysis of the galaxy cluster A2670, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A combined X-ray and optical analysis of the galaxy cluster A2670 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-806877