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Astrometry of the open cluster NGC 2324

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Abstract

New proper motion membership probabilities are given for stars in the region of the cluster NGC 2324. The space density distribution and the luminosity function are discussed. A comparison with previous investigations is presented.

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References

  • Aiad, A.: 1986a,Bull. Fac. Sci. Cairo Univ. 54, 745.

    Google Scholar 

  • Aiad, A.: 1986b,Bull. Fac. Sci. Cairo Univ. 54, 753.

    Google Scholar 

  • Barkhatova, K. A.: 1963,Sb. Ural Univ 1, 3.

    Google Scholar 

  • Becker, W.: 1960,Z. Astrophys. 51, 45.

    Google Scholar 

  • Gehzloun, G.: 1977,Ann. Obs. Alger, Tome V (Fascicule 4).

  • Jones, B. F.: 1970,Astron. J. 75, 563.

    Google Scholar 

  • Jones, B. F. and Kyle Cudworth: 1983,Astron. J. 88, 215.

    Google Scholar 

  • Limber, D. N.: 1962a,Astrophys. J. 135, 16.

    Google Scholar 

  • Rahim, M. and Hassan, S.: 1967,Helwan Obs. Bull., No. 71.

  • Van Altena, W. F. and Jones, B. F.: 1972,Astron. Astrophys. 20, 425.

    Google Scholar 

  • Van den Bergh, S. and Sher, D.: 1960,Publ. David Dunlap Obs. 2, 203.

    Google Scholar 

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Marie, M. Astrometry of the open cluster NGC 2324. Astrophys Space Sci 201, 71–77 (1993). https://doi.org/10.1007/BF00626975

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  • DOI: https://doi.org/10.1007/BF00626975

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