No CrossRef data available.
Article contents
An Automated Method of General Star Counts For Dark Clouds
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
An automated method of general star counts has been developed for the purpose of deriving the distributions of extinction of large dark clouds. The result of the application to the Southern Coalsack is given.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 78: Astronomy with Schmidt-type telescopes , 1984 , pp. 329 - 332
- Copyright
- Copyright © Reidel 1984
References
Buonanno, R. and Corsi, C. E., 1978, in Proceedings of the 5th Colloquium on Astrophysics, Trieste, International Workshop in Image Processing in Astronomy., ed. Sedmak, G. , Capaccioli, M. and Allen, R. J. (Observatorio Astronomico di Trieste, Trieste), pp.354–359.Google Scholar
Saito, T., Ohtani, H. and Tomita, Y., Publ. Astron. Soc. Japan, 33, 327, 1981, pp.327–340.Google Scholar
Tapia, S., 1973, in IAU Symposium 52, Interstellar Dust and Related Topics, ed. Greenberg, J. M. and Van de Hulst, H. C. (Reidel, Dordrecht), p.43.Google Scholar