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Dust, Star, and Hydrogen Distributions in the Orion Association

Published online by Cambridge University Press:  14 August 2015

Syuzo Isobe
Syuzo Isobe*
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, Mitaka, Tokyo

Abstract

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From the star counts on the Palomar Sky Survey prints, dust and star distributions in the Orion Association are studied. The Hydrogen distribution in the same region is obtained from an Hα photograph. It is found that a considerable part of the interstellar absorption on the line of sight is due to the circumstellar dust grains in the Orion Association.

Type
Part VIII Dust and H II Regions
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973 , pp. 433 - 444
Copyright
Copyright © Reidel 1973 

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