Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....92..189c&link_type=abstract
Astronomy and Astrophysics, vol. 92, no. 1-2, Dec. 1980, p. 189-195. In French.
Astronomy and Astrophysics
Astrophysics
4
Galactic Rotation, Spiral Galaxies, Abundance, Angular Velocity, Astronomical Photometry, Astronomical Spectroscopy, H Ii Regions, Mass Distribution, Nebulae
Scientific paper
Spectra taken with nebular spectrographs of the Haute Provence Observatory (35 A/mm in the 6450-6800 A range and 92 A/mm in the 3700-5100 A range) yield a linear rotation curve for the peculiar edge-on galaxy NGC 2976; the curve is slightly steeper for the NW region than for the SE one; this leads to a very small mass of two billion solar masses. This mass and the low luminosity (420 million solar luminosities) classify this galaxy as a late spiral. It is found that NGC 2976 as a whole contains large H II regions of moderate excitation.
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