Abstract
In the present paper various observational data are used to compare seven most common models proposed to describe the behaviour of the interstellar extinction in different parts of the sky. The data for field stars, open and globular clusters are used to select the most adequate model at different distances and for different directions in the Galaxy. The results of this study allow to select the best models for particular distances and directions. They also make it possible to propose a synthesized model describing the interstellar extinction.
Similar content being viewed by others
References
Adelman, S.J., Pyper, D.M. and White, R.E.: 1980, ApJ Suppl. Ser. 43, 491.
Arenou, F., Grenon, M. and Gomez A.: 1992, A&A 258, 104.
de Vaucouleurs, G., de Vaucouleurs, A. and Corwin, H.G.: 1976, Second Reference Catalogue of Bright Galaxies, Austin: University of Texas Press.
Djorgovski, S.: 1993, ESO Sci. Preprint 932, 39.
Djorgovski, S. and Meylan, G.: 1993, ESO Sci. Preprint 932, 3.
FitzGerald, P.M.: 1968, AJ 73, 983.
Krautter, J.: 1980, A&A Suppl. Ser. 39, 167.
Loktin, A.V., Matkin, N.V. and Gerasimenko T.P.: 1992, The Catalogue of Galactic Cluster Parameters from UBV-Data. Centre de Données astronomiques de Strasbourg.
Neckel, Th. and Klare, G.: 1980, A&A Suppl. Ser. 42, 251.
Pandey, A.K. and Mahra, H.S.: 1987, MNRAS 226, 635.
Parenago, P.P.: 1940, Astron. Zh. 17, 3.
Peterson, C.J.: 1993, ESO Sci. Preprint 932, 13.
Rauch, T., Heber, U., Hunger, K., Werner, K. and Neckel, T.: 1991, A&A 241, 457.
Reed, C.B.: 1993, PASP 105, 1465.
Sandage, A.: 1972, ApJ 178, 1.
Sharov, A.S.: 1963, Astron. Zh. 40, 900.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Malkov, O., Kilpio, E. A Synthetic Map of the Galactic Interstellar Extinction. Astrophysics and Space Science 280, 115–118 (2002). https://doi.org/10.1023/A:1015526811574
Issue Date:
DOI: https://doi.org/10.1023/A:1015526811574