Abstract
A ring of compact radio continuum sources was found at l = 24 °. 6 b = 0 °. 0, which we call the Scutum ring. Radio continuum, HI line, and CO line observations are suggested that it is a star-forming region triggered by an expanding diffuse HII region.
NRO, a branch of the Tokyo Astronomical Observatory, University of Tokyo, is a cosmic radio observing facility open for outside users.
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References
Dame, T. M.: 1984, NASA Technical Paper, No. 2288.
Downes, D., Wilson, T. L., Bieging, J., Wink, J.: 1980, Astron. Astrophys. Suppl 40, 379.
Elmegreen, B. G. and Lada, C. J.: 1911, Astrophys. J. 214, 725.
Handa, T., Sofue, Y., Reich, W., Fürst, E., Suwa, L, and Fukui, Y.: 1985, Publ. Astron. Soc. Japan (submitted).
Sofue, Y., Hirabayashi, H., Akabane, K., Inoue, M., Handa, T., and Nakai, N.: 1984, Publ. Astron. Soc. Japan 36, 287.
Westerhout, G. and Wendlandt, H.-U.: 1982, Astron. Astrophys. Suppl. 49, 143.
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© 1986 D. Reidel Publishing Company
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Handa, T., Sofue, Y. (1986). The Scutum Ring of Hii Regions. In: Kitamura, M., Budding, E. (eds) Third Asian-Pacific Regional Meeting of the International Astronomical Union. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4630-9_29
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DOI: https://doi.org/10.1007/978-94-009-4630-9_29
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-8558-8
Online ISBN: 978-94-009-4630-9
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