Dark matter content in globular cluster NGC 6397

Jihye Shin, Sungsoo S. Kim, Young-Wook Lee

Research output: Contribution to journalArticle

5 Citations (Scopus)

Abstract

We trace the dynamical evolution of dark matter (DM) content in NGC 6397, one of the native Galactic globular clusters (GCs). The relatively strong tidal field (Galactocentric radius of ~ 6 kpc) and short relaxation timescale (~ 0.3 Gyr) of the cluster can cause a significant amount of DM particles to evaporate from the cluster in the Hubble time. Thus, the cluster can initially contain a non-negligible amount of DM. Using the most advanced Fokker-Planck (FP) method, we calculate the dynamical evolution of GCs for numerous initial conditions to determine the maximum initial DM content in NGC 6397 that matches the present-day brightness and velocity dispersion profiles of the cluster. We find that the maximum allowed initial DM mass is slightly less than the initial stellar mass in the cluster. Our findings imply that NGC 6397 did not initially contain a significant amount of DM, and is similar to that of NGC 2419, the remotest and the most massive Galactic GC.

Original languageEnglish
Pages (from-to)173-181
Number of pages9
JournalJournal of the Korean Astronomical Society
Volume46
Issue number4
DOIs
Publication statusPublished - 2013 Sep 3

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globular clusters
dark matter
stellar mass
brightness
timescale
radii
causes
profiles

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics

Cite this

Shin, Jihye ; Kim, Sungsoo S. ; Lee, Young-Wook. / Dark matter content in globular cluster NGC 6397. In: Journal of the Korean Astronomical Society. 2013 ; Vol. 46, No. 4. pp. 173-181.
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Dark matter content in globular cluster NGC 6397. / Shin, Jihye; Kim, Sungsoo S.; Lee, Young-Wook.

In: Journal of the Korean Astronomical Society, Vol. 46, No. 4, 03.09.2013, p. 173-181.

Research output: Contribution to journalArticle

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