Rotation of Stars and Gas in M82

Details Rotation of Stars and Gas in M82 Rotation of Stars and Gas in M82

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...272...98m&link_type=abstract

Astronomy and Astrophysics, Vol.272, NO. 1/MAYI, P. 98, 1993

Astronomy and Astrophysics

Astrophysics

29

Scientific paper

New observations of near IR emission and absorption lines along M 82's major axis yield radial velocity-position curves that differ markedly from those derived from lines at visible wavelengths. For the central disk we find identical rotation for the gas and the stars, contrary to earlier results. The rotation derived from emission and absorption lines at visible wavelengths refer to outer regions of the galaxy since at these wavelengths the central disk is obscured by dust.

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