On the nature of the stellar population in the nucleus of the SD galaxy NGC 7793

Details On the nature of the stellar population in the nucleus of the SD galaxy NGC 7793 On the nature of the stellar population in the nucleus of the SD galaxy NGC 7793

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.201p..49d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 201, Nov. 1982, p. 49P-55P.

Other

10

A Stars, Chemical Composition, Galactic Evolution, Galactic Nuclei, Spiral Galaxies, Star Distribution, Abundance, Calcium, Hydrogen, Late Stars, Main Sequence Stars, Spectral Energy Distribution, Spectral Line Width

Scientific paper

Profiles and equivalent widths of hydrogen, Ca+ and some
other lines imply that the blue-violet spectrum of the nucleus of this
late-type spiral is dominated by A or early F stars near the main
sequence and not by a mixture of globular cluster-like populations.

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