Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...353...90w&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 353, April 10, 1990, p. 90-102. Research supported by NASA and NSERC.
Astronomy and Astrophysics
Astrophysics
6
Galactic Rotation, Luminosity, Spiral Galaxies, Virgo Galactic Cluster, Astronomical Photometry, Brightness Distribution, Charge Coupled Devices, Emission Spectra, Velocity Distribution
Scientific paper
Optical rotation curves are presented for the innermost portions of nine spiral galaxies in the Virgo Cluster. The emission-line (H-alpha and forbidden N II) velocity data are to be used in combination with new CCD photometry to construct luminosity-velocity diagrams, in a continuing investigation of an apparent initial linear branch and its potential as a distance indicator. Compared to recent H I data, the present optical rotation curves generally show systematically steeper inner gradients. This effect is ascribed to the poorer resolution of the H I data and/or to holes in the gas distribution.
Fahlman Gregory G.
Madore Barry F.
Woods David
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