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- W2048809918 abstract "The structure of a very bright (MV = -10.9) globular cluster in NGC 1023 is analyzed on two sets of images taken with the Hubble Space Telescope. From careful modeling of King profile fits to the cluster image, a core radius of rc = 0.55 ± 0.1 pc, effective radius Re = 3.7 ± 0.3 pc, and a central surface brightness of μ0(V) = 12.9 ± 0.5 mag arcsec-2 are derived. This makes the cluster much more compact than ω Cen, but very similar to the brightest globular cluster in M31, G1 (= Mayall II). The cluster in NGC 1023 appears to be very highly flattened with an ellipticity of ≈ 0.37, even higher than for ω Cen and G1, and similar to the most flattened clusters in the Large Magellanic Cloud." @default.
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- W2048809918 date "2001-10-01" @default.
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- W2048809918 title "A G1-like Globular Cluster in NGC 1023" @default.
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- W2048809918 doi "https://doi.org/10.1086/323138" @default.
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