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A study of the young open cluster NGC 6611

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Abstract

Photoelectric magnitudes and colours in theUBV system have been determined for 50 stars in NGC 6611. The reddening value varies across the cluster fromE(B-V)=0m58 toE(B-V)=1m21. The distance modulus to the cluster is estimated at 12m5±0m2. It is found that cluster stars are not of the same age. The cluster luminosity function is compared with the general and initial luminosity functions.

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References

  • Barbaro, G., Dallaporta, N. and Fabris, G.: 1969,Astrophys. Space Sci. 3, 123.

    Google Scholar 

  • Becker, W. and Fenkart, R.: 1970, in W. Becker and G. Contopoulos (eds), ‘The Spiral Structure of Our Galaxy’,IAU Symp. 38, 205.

  • Becker, W. and Fenkart, R.: 1971,Astron. Astrophys. Suppl. 4, 241.

    Google Scholar 

  • Burki, G.: 1975,Astron. Astrophys. 43, 37.

    Google Scholar 

  • Conti, P. S. and Alschuler, W. R.: 1971,Astrophys. J. 170, 325.

    Google Scholar 

  • Golay, M.: 1974,Introduction to Astronomical Photometry, D. Reidel Publ. Co., Dordrecht, p. 138.

    Google Scholar 

  • Hiltner, W. A. and Morgan, W. W.: 1969,Astron. J. 74, 1152.

    Google Scholar 

  • Hoag, A. A., Johnson, H. L., Iriarte, B., Mitchell, R. I., Hallam, K. L., and Sharpless, S.: 1961.Publ. U.S. Naval Obs. (2nd Series),17, Part 7, p. 432.

    Google Scholar 

  • Kamp, L. W.: 1974,Astron. Astrophys. Suppl 16, 1.

    Google Scholar 

  • McNamara, B. J. and Sanders, W. L.: 1976,Astron. Astrophys. 52, 53.

    Google Scholar 

  • Mermilliod, J. C.: 1976,Astron. Astrophys. Suppl. 24, 159.

    Google Scholar 

  • Moffat, A. F. J. and Schmidt-Kaler, Th.: 1976,Astron. Astrophys. 48, 115.

    Google Scholar 

  • Sagar, R. and Joshi, U. C.: 1978a,Bull. Astron. Soc. India 6, 12.

    Google Scholar 

  • Sagar, R. and Joshi, U. C.: 1978b,Bull. Astron. Soc. India 6, 37.

    Google Scholar 

  • Sagar, R. and Joshi, U. C.: 1978c,Monthly Notices Roy. Astron. Soc. 184, 467.

    Google Scholar 

  • Schmidt-Kaler, Th.: 1965, ‘Physical Parameters and Two-Parameter diagrams of the Stars’, in Landolt-Bornstein,Numerical Data and Functional Relationship, Science and Technology, Group VI, I, H. H. Voigt (ed.), p. 284.

  • van Schewick, H.: 1962,Veröffentl. Univ. Stenw. Bonn 62, 3.

    Google Scholar 

  • Walker, M. F.: 1961,Astrophys. J. 133, 438.

    Google Scholar 

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Sagar, R., Joshi, U.C. A study of the young open cluster NGC 6611. Astrophys Space Sci 66, 3–12 (1979). https://doi.org/10.1007/BF00648356

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  • DOI: https://doi.org/10.1007/BF00648356

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