Abstract
It has been found that certain optical properties of interstellar grains obtained by Hayakawaet al. (1969) from their study of the diffuse radiation of the Galaxy in far UV are not in reality consistent with the more accurate theoretical calculations of diffuse radiation for the model of the Galaxy used by Hayakawaet al. in their work. A more complex model of the Galaxy may be required for interpretation of observations in far UV.
Similar content being viewed by others
References
Greenberg, J. M. and Shah, G. A.: 1969,Physica 41, 92.
Hayakawa, S., Yamashita, K., and Yoshioka, S.: 1969,Astrophys. Space Sci. 5, 493.
Henyey, L. G. and Greenstein, Y. L.: 1941,Astrophys. J. 93, 70.
RoŽkovskij, D. A.: 1969,Westnik Acad. of Sci. Kazakhskoi S.S.R., No. 7.
RoŽkovskij, D. A. and Matjagin, V. S.:Trudy Astrophys. Inst. Acad. of Sci. Kazakh S.S.R. (in press).
Van de Hulst, H. C. and De Jong, T.: 1969,Physica 41, 151.
Author information
Authors and Affiliations
Additional information
Receipt delayed by postal strike in Great Britain.
Rights and permissions
About this article
Cite this article
Rožkovskij, D.A., Matjagin, V.S. On the diffuse radiation of the Galaxy in far UV according to the investigations by S. Hayakawa, K. Yamashita and S. Yoshioka. Astrophys Space Sci 12, 204–207 (1971). https://doi.org/10.1007/BF00656150
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00656150