Method for determination of cluster radius from radial density profile
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We propose the numerical method for determining the radius of a star cluster using its radial surface density profile. The method realizes the algorithm of an eye estimate but minimizes a subjectivity; its result is in a good agreement with the eye estimate of the radius for the open cluster NGC 2516.
2017 ◽
Vol 34
(2)
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pp. 83-97
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1998 ◽
Vol 248
(5-6)
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pp. 400-404
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1982 ◽
Vol 17
(1)
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pp. 53-61
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