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Emission line velocity field in the central region of M82

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Abstract

Velocity field in the central region of M82 has drawn in detail mainly from Hα. This velocity field is consistent with that of Neii 12.8 μm except for the region near a huge dust lane, and it cannot be explained by pure rotation around the galactic center. Origin of peculiarities of the velocity field is briefly discussed.

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Authors and Affiliations

  1. Department of Astronomy, Faculty of Science, University of Kyoto, Kyoto, Japan

    Minoru Sasaki & Mamoru Saito

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  1. Minoru Sasaki
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  2. Mamoru Saito
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Sasaki, M., Saito, M. Emission line velocity field in the central region of M82. Astrophys Space Sci 119, 181–184 (1986). https://doi.org/10.1007/BF00648842

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  • DOI: https://doi.org/10.1007/BF00648842

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