Globular Clusters around Galaxies in Groups
2002 ◽
Vol 207
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pp. 342-344
We have obtained deep photometry of NGC 1199 (in HCG 22) and NGC 6868 (in the Telescopium group). Both galaxies are the optically brightest galaxies of their groups. Our analysis of B and R images taken with the Keck II and the VLT/ESO telescopes, detected a population of globular clusters around both galaxies, with total specific frequencies SN = 1.7 ± 0.6 for NGC 1199 and SN = 1.3 ± 0.6 for NGC 6868. The color distributions of the globular cluster systems shows bimodal peaks centered at (B - R)0 = 1.13 ± 0.10 and 1.42 ± 0.10 (NGC 1199) and (B - R)0 = 1.12 ± 0.10 and 1.42 ± 0.10 (NGC 6868).
2010 ◽
pp. no-no
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1983 ◽
Vol 100
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pp. 359-364
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2007 ◽
Vol 3
(S246)
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pp. 394-402
1995 ◽
Vol 164
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pp. 441-442
2002 ◽
Vol 207
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2002 ◽
Vol 207
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pp. 281-286
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2002 ◽
Vol 207
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pp. 333-335
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2009 ◽
Vol 396
(2)
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pp. 1075-1085
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2010 ◽
Vol 409
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pp. 447-448
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