Abstract
PAGEL1 has proposed a new method for the determination of the intrinsic and interstellar reddening for peculiar objects which is based on the intensities of the forbidden lines of ionized iron, and has applied the method to the interesting southern object Eta Carinae.
Similar content being viewed by others
References
Pagel, B. E. J., Nature, 221, 325 (1969).
Thackeray, A. D., Mon. Not. Roy. Astro. Soc., 135, 51 (1967).
Garstang, R. H., Mon. Not. Roy. Astro. Soc., 124, 321 (1962).
Rodgers, A. W., and Searle, L., Mon. Not. Roy. Astro. Soc., 135, 99 (1967).
Aller, L. H., and Dunham, T., Astrophys. J., 146, 126 (1966).
Aller, L. H., Proc. US Nat. Acad. Sci., 55, 671 (1966).
Seaton, M. J., Rep. Prog. Phys., 23, 322 (1960).
Warner, B., Mem. Roy. Astro. Soc., 70, 165 (1967).
Warner, B., Mon. Not. Roy. Astro. Soc., 133, 389 (1966).
Merrill, P. W., Lines of the Chemical Elements in Astronomical Spectra (Carnegie Institution of Washington, 1958).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
LAMBERT, D. Intrinsic Reddening of Eta Carinae. Nature 223, 726–727 (1969). https://doi.org/10.1038/223726a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/223726a0
- Springer Nature Limited
This article is cited by
-
The nature of ? carinae
Astrophysics and Space Science (1990)