Emission line velocity field in the central region of M82

Details Emission line velocity field in the central region of M82 Emission line velocity field in the central region of M82

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..181s&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

Emission Spectra, Galactic Nuclei, H Alpha Line, Irregular Galaxies, Radial Velocity, Galactic Rotation, Infrared Spectra, Interstellar Matter

Scientific paper

Velocity field in the central region of M82 has drawn in detail mainly
from Hα. This velocity field is consistent with that of Ne II 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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