Inference of black-hole mass fraction in Galactic globular clusters - A multi-dimensional approach to break the initial-condition degeneracies

Home

All issues

Volume 690 (October 2024)

A&A, 690 (2024) A179

Full HTML

Open Access

Table B.1

Properties of the sample of 21 clusters analyzed in this study with FoV larger than R_hl.

Cluster	Δ_obs(< R_hl)	σ_μ (< 0.2R_hl)/σ_μ(R_hl)
NGC 1261	${0.043}_{- 0.002}^{+ 0.002}$ $\[0.043_{-0.002}^{+0.002}\]$	1.11 ± 0.04
NGC 2298	${0.044}_{- 0.003}^{+ 0.004}$ $\[0.044_{-0.003}^{+0.004}\]$	−
NGC 4590	${0.049}_{- 0.002}^{+ 0.002}$ $\[0.049_{-0.002}^{+0.002}\]$	−
NGC 4833	${0.046}_{- 0.002}^{+ 0.002}$ $\[0.046_{-0.002}^{+0.002}\]$	−
NGC 5024	${0.049}_{- 0.001}^{+ 0.001}$ $\[0.049_{-0.001}^{+0.001}\]$	1.20 ± 0.05
NGC 5904	${0.036}_{- 0.001}^{+ 0.001}$ $\[0.036_{-0.001}^{+0.001}\]$	1.16 ± 0.02
NGC 5927	${0.038}_{- 0.002}^{+ 0.001}$ $\[0.038_{-0.002}^{+0.001}\]$	1.05 ± 0.04
NGC 5986	${0.039}_{- 0.002}^{+ 0.001}$ $\[0.039_{-0.002}^{+0.001}\]$	−
NGC 6144	${0.029}_{- 0.003}^{+ 0.003}$ $\[0.029_{-0.003}^{+0.003}\]$	−
NGC 6171	${0.044}_{- 0.003}^{+ 0.003}$ $\[0.044_{-0.003}^{+0.003}\]$	−
NGC 6205	${0.031}_{- 0.001}^{+ 0.001}$ $\[0.031_{-0.001}^{+0.001}\]$	1.21 ± 0.04
NGC 6218	${0.046}_{- 0.002}^{+ 0.002}$ $\[0.046_{-0.002}^{+0.002}\]$	−
NGC 6304	${0.064}_{- 0.002}^{+ 0.002}$ $\[0.064_{-0.002}^{+0.002}\]$	1.15 ± 0.08
NGC 6535	${0.042}_{- 0.007}^{+ 0.006}$ $\[0.042_{-0.007}^{+0.006}\]$	−
NGC 6584	${0.023}_{- 0.003}^{+ 0.002}$ $\[0.023_{-0.003}^{+0.002}\]$	−
NGC 6637	${0.055}_{- 0.002}^{+ 0.002}$ $\[0.055_{-0.002}^{+0.002}\]$	1.26 ± 0.06
NGC 6717	${0.060}_{- 0.006}^{+ 0.006}$ $\[0.060_{-0.006}^{+0.006}\]$	−
NGC 6723	${0.033}_{- 0.002}^{+ 0.002}$ $\[0.033_{-0.002}^{+0.002}\]$	−
NGC 6779	${0.041}_{- 0.002}^{+ 0.002}$ $\[0.041_{-0.002}^{+0.002}\]$	−
NGC 6934	${0.054}_{- 0.002}^{+ 0.002}$ $\[0.054_{-0.002}^{+0.002}\]$	1.04 ± 0.05
NGC 6981	${0.029}_{- 0.003}^{+ 0.002}$ $\[0.029_{-0.003}^{+0.002}\]$	−

Notes. Δ_obs(< R_hl) and velocity dispersion ratio for the clusters with FoV coverage of at least one R_hl. The velocity dispersion was computed directly from individual stars within 0.2R_hl and around R_hl. Only clusters with at least 100 stars within these ranges were considered.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.