Abstract
The calibrated Hα-map of S237 and its profiles in section through the nebular center are presented. The core-envelope structure and central open shell appearance are noticed. Physical parameters such as emission measure and mass of ionized gas are deduced and compared with results of radio observations.
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Chopinet, M., Georgelin, Y. M. and Lortet-Zuckermann, M. C.: 1973,Astron. Astrophys. 29, 225.
Crampton, D., Georgelin, Y. M. and Georgelin, Y. P.: 1978,Astron. Astrophys. 66, 1.
Hoag, A. A., Johnson, H. L., Iriate, B., Mitchell, R. I., Hallam, K. L. and Sharpless, S.: 1961, Publ. U.S. Naval Observatory, XVII.
Ishida, K. and Kawajiri, N.: 1968,Publ. Astron. Soc. Japan 20, 95.
Israel, F. P.: 1977,Astron. Astrophys. 61, 377.
Mizuno, S.: 1981, Thesis, Kyoto University (in preparation).
Pyatunina, T. B.: 1980,Astrophys. Space Sci. 67, 173.
Sharpless, S.: 1959,Astrophys. J. Suppl. 4, 257.
Silverglate, P. R. and Terzian, Y.: 1979,Astrophys. J. Suppl. 39, 157.
Takase, B., Ishida, K., Shimizu, M., Maehara, H., Hamajima, K., Noguchi, T. and Ohashi, M.: 1977,Ann. Tokyo Astron. Obs., 2nd Ser. XVI, No. 2, 74.
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Mizuno, S., Sakka, K., Sasaki, T. et al. The calibrated map of the HII region S237 in Hα emission. Astrophys Space Sci 78, 235–242 (1981). https://doi.org/10.1007/BF00654036
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DOI: https://doi.org/10.1007/BF00654036