The morphology of Sersic-Pastoriza galaxies

Details The morphology of Sersic-Pastoriza galaxies The morphology of Sersic-Pastoriza galaxies

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3098..245y&link_type=abstract

In NASA, Marshall Space Flight Center, Paired and Interacting Galaxies: International Astronomical Union Colloquium No. 124 p 24

Astronomy and Astrophysics

Astronomy

Galaxies, Morphology, Neutral Gases, Supernova Remnants, Astronomy, Hydrogen, Populations, Spectroscopy

Scientific paper

The authors present the preliminary results of their radio-continuum and
neutral hydrogen observations of Sersic-Pastoriza (S-P) galaxies. They
show that the central regions contain a population of compact features
thought to be young supernova remnants (SNRs) and discuss the overall
morphology of the nuclei.

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