Supermassive disk galaxies

Details Supermassive disk galaxies Supermassive disk galaxies

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991msngr..63...50b&link_type=abstract

ESO Messenger (ISSN 0722-6691), no. 63, p. 50-52.

Physics

Disk Galaxies, Galactic Mass, H Beta Line, Rotational Spectra, Cosmic Gases, Data Reduction, Galactic Bulge

Scientific paper

In order to investigate the properties of supermassive disk galaxies (SDGs), an extensive optical survey of SDG candidates in the Southern Hemisphere was performed with the 2.2-m ESO/MPI telescope at La Silla. The question of whether SDGs have in general an unusually high content of dark matter in the inner regions or, perhaps, an unusual stellar population is addressed. It is suggested that SDGs are formed as the result of a series of accretion events, possibly induced also by the progressive deepening of the galaxy potential well.

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