期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 401, 期 1, 页码 533-546出版社
WILEY-BLACKWELL PUBLISHING, INC
DOI: 10.1111/j.1365-2966.2009.15678.x
关键词
globular clusters: general; galaxies: individual: M31
资金
- European Commission [MCEXT-CT-2005-025869]
- STFC
- [GN-2007B-Q-58]
- STFC [ST/H004165/1, PP/E00105X/1, ST/G001979/1, PP/C002229/1, ST/H001972/1, ST/H004157/1, ST/H001913/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/H004165/1, PP/E00105X/1, ST/G001979/1, PP/C002229/1, ST/H00243X/1, ST/H001913/1, ST/H004157/1, ST/H001972/1] Funding Source: researchfish
We report on deep imaging of a remote M31 globular cluster, MGC1, obtained with Gemini/GMOS. Our colour-magnitude diagram for this object extends similar to 5 mag below the tip of the red-giant branch and exhibits features consistent with an ancient metal-poor stellar population, including a long, well-populated horizontal branch. The red-giant branch locus suggests MGC1 has a metal abundance [M/H] approximate to -2.3. We measure the distance to MGC1 and find that it lies similar to 160 kpc in front of M31 with a distance modulus mu = 23.95 +/- 0.06. Combined with its large projected separation of R(p) = 117 kpc from M31, this implies a deprojected radius of R(gc) = 200 +/- 20 kpc, rendering it the most isolated known globular cluster in the Local Group by some considerable margin. We construct a radial brightness profile for MGC1 and show that it is both centrally compact and rather luminous, with M(V) = -9.2. Remarkably, the cluster profile shows no evidence for a tidal limit and we are able to trace it to a radius of at least 450 pc, and possibly as far as similar to 900 pc. The profile exhibits a power-law fall-off with exponent gamma = -2.5, breaking to gamma = -3.5 in its outermost parts. This core-halo structure is broadly consistent with expectations derived from numerical models, and suggests that MGC1 has spent many gigayears in isolation.
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