Abstract
12C0(J = 1-0) observations of the central region of NGC4258 at a resolution of 17” revealed a high-density concentration of molecular gas toward the center. The molecular clump lies on a central depression in the HI bar. No clear interaction of the molecular gas with the continuum anomalous arms has been found.
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References
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© 1989 International Astronomical Union
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Sofue, Y. (1989). CO Observations of the Central Region of NGC4258. In: McNally, D. (eds) Highlights of Astronomy. International Astronomical Union / Union Astronomique Internationale, vol 8. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0977-9_97
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DOI: https://doi.org/10.1007/978-94-009-0977-9_97
Publisher Name: Springer, Dordrecht
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