{[ promptMessage ]}

Bookmark it

{[ promptMessage ]}

Velocity dispersion - Velocity dispersion this is a...

Info icon This preview shows page 1. Sign up to view the full content.

View Full Document Right Arrow Icon
Velocity dispersion: this is a total-mass indicator, and is generally largest for rich, regular, relaxed clusters. An unbiased (or maybe only slightly biased) virial mass estimator is given by Heisler et al 1985 (ApJ 298, 8) as where V i is the radial velocity of galaxy i with respect to the cluster mean, R is the projected distance from the cluster center, α ~1.5 is a fudge factor accounting for the fact the the center must be determined from the galaxy positions themselves, and f PM depends on the typical orbital shape; it has values 32/ π for isotropically distributed orbits and 64/ π for purely radial orbits. See also the discussion of mass estimators by Postman, Huchram and Geller 1988 (AJ 95, 267). One might well ask whether and how clusters blend into groups and any larger structure. Peebles championed the use of a correlation function as a statistical probe for this (see his book Large- Scale Structure of the Universe , Princeton 1980). The correlation function ξ measures the
Image of page 1
This is the end of the preview. Sign up to access the rest of the document.

{[ snackBarMessage ]}