Abstract
From a new infrared photometry of the globular cluster M10 its interstellar extinction and distance modulus are discussed. This is done by comparison with the well-studied clusters M3, M13, and M92. Final values ofE(B-V)=0.17±0.05 and (M v-V)=14.0±0.3 are proposed. The dependence on metallicity of these values is briefly discussed.
Similar content being viewed by others
References
Frogel, J. A., Persson, S. E., and Cohen, J. G.: 1981,Astrophys. J. 246, 842.
Frogel, J. A., Persson, S. E., and Cohen, J. G.: 1983a,Astrophys. J. Suppl. Ser. 53, 713.
Frogel, J. A., Persson, S. E., and Cohen, J. G.: 1983b,Astrophys. J. 275, 773.
Harris, W. E., Racine, R., and Roux, J.: 1976,Astrophys. J. Suppl. Ser. 31, 13.
Martinez Roger, C.: 1987,Astron. Astrophys. 171, 77.
Sandage, A.: 1970,Astrophys. J. 162, 841.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Arribas, S., Martinez Roger, C., Paez, E. et al. The interstellar extinction and distance modulus to M10 from infrared photometry. Astrophys Space Sci 169, 45–47 (1990). https://doi.org/10.1007/BF00640684
Issue Date:
DOI: https://doi.org/10.1007/BF00640684