Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-10-27
Astrophys.J. 585 (2003) 598-601
Astronomy and Astrophysics
Astrophysics
4 pages, 4 figures, submitted to ApJ
Scientific paper
10.1086/345991
It has recently come to our attention that there are axis scale errors in three of the figures of Dull et al. (1997, hereafter D97). D97 presented Fokker-Planck models for the collapsed-core globular cluster M15 that include a dense, centrally concentrated population of neutron stars and massive white dwarfs, but do not include a central black hole. In this Addendum, we present corrected versions of Figures 9, 10, and 12, and an expanded version of Figure 6. This latter figure, which shows the full run of the velocity dispersion profile, indicates that the D97 model predictions are in good agreement with the moderately rising HST-STIS velocity dispersion profile for M15 reported by Gerssen et al. (2002, astro-ph/0209315). Thus, a central black hole is not required to fit the new STIS velocity measurements, provided that there is a sufficient population of neutron stars and massive white dwarfs. This conclusion is consistent with the findings of Gerssen et al. (2002, astro-ph/0210158), based on a reapplication of their Jeans equation analysis using the corrected mass-to-light profile (Figure 12) for the D97 models.
Callanan Paul J.
Charles Phil A.
Cohn Haldan N.
Dull James D.
Lugger Phyllis Minnie
No associations
LandOfFree
Addendum: "The Dynamics of M15: Observations of the Velocity Dispersion Profile and Fokker-Planck Models" (ApJ, 481, 267 [1997]) 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 Addendum: "The Dynamics of M15: Observations of the Velocity Dispersion Profile and Fokker-Planck Models" (ApJ, 481, 267 [1997]), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Addendum: "The Dynamics of M15: Observations of the Velocity Dispersion Profile and Fokker-Planck Models" (ApJ, 481, 267 [1997]) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-49220