2004MNRAS.348..589C


Query : 2004MNRAS.348..589C

2004MNRAS.348..589C - Mon. Not. R. Astron. Soc., 348, 589-598 (2004/February-3)

The statistical analysis of star clusters.

CARTWRIGHT A. and WHITWORTH A.P.

Abstract (from CDS):

We review a range of statistical methods for analysing the structures of star clusters, and derive a new measure Q, which both quantifies and distinguishes between a (relatively smooth) large-scale radial density gradient and multiscale (fractal) subclustering.
The distribution of separations p(s) is considered, and the normalized correlation length {bar}s (i.e. the mean separation between stars, divided by the overall radius of the cluster) is shown to be a robust indicator of the extent to which a smooth cluster is centrally concentrated. For spherical clusters having volume-density n ∝r –α (with α between 0 and 2) {bar}s decreases monotonically with α, from ∼0.8 to ∼0.6. Since {bar}s reflects all star positions, it implicitly incorporates edge effects. However, for fractal star clusters (with fractal dimension D between 1.5 and 3) {bar}s decreases monotonically with D (from ∼0.8 to ∼0.6). Hence {bar}s, on its own, can quantify, but cannot distinguish between, a smooth large-scale radial density gradient and multiscale (fractal) subclustering.
The minimal spanning tree (MST) is then considered, and it is shown that the normalized mean edge length {bar}m [i.e. the mean length of the branches of the tree, divided by (NtotalA)1/2/ (Ntotal - 1), where A is the area of the cluster and Ntotal is the number of stars] can also quantify, but again cannot on its own distinguish between, a smooth large-scale radial density gradient and multiscale (fractal) subclustering.
However, the combination Q = {bar}s/ {bar}m does both quantify and distinguish between a smooth large-scale radial density gradient and multiscale (fractal) subclustering. IC348 has Q = 0.98 and ρ Ophiuchus has Q = 0.85, implying that both are centrally concentrated clusters with, respectively, α≃ 2.2±0.2 and α≃ 1.2 ± 0.3. Chamaeleon and IC2391 have Q = 0.67 and 0.66, respectively, implying mild substructure with a notional fractal dimension D ≃ 2.25±0.25. Taurus has even more substructure, with Q = 0.45 implying D '≃ 1.55±0.25. If the binaries in Taurus are treated as single systems, Q increases to 0.58 and D ' increases to 1.9±0.2.

Abstract Copyright: 2004 RAS

Journal keyword(s): open clusters and associations: general

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 IC 348 OpC 03 44 31.1 +32 10 02           ~ 1476 1
2 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
3 IC 2391 OpC 08 41 17.5 -53 03 00           ~ 871 0
4 NAME Chamaeleon Region SFR 11 55 -78.0           ~ 887 0
5 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1

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