Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983msngr..31....5l&link_type=abstract
ESO Messenger (ISSN 0722-6691), March 1983, p. 5-7.
Physics
Barred Galaxies, Galactic Nuclei, Galactic Structure, Radio Galaxies, Emission Spectra, Galactic Clusters, Galactic Rotation, H Alpha Line, H Ii Regions, Radial Velocity, Southern Sky, Supernova Remnants
Scientific paper
The barred galaxy NGC 1365 was chosen for study with the European Southern Observatory's 3.6 m telescope because its orientation is ideal for kinematic investigations, its structure is rich in interstellar matter, and earlier observations have indicated that the strong emission line spectrum from the nuclear region might be due to violet noncircular motions. The nuclear region of NGC 1365 is penetrated by a strong dust lane and contains a number of hot spots and H II regions situated along the nearer arm of a small nuclear spiral. Attention is given to spectrographic measurements of the velocity field outside the nuclear region, together with VLA observations of the galaxy which show no radio emission from the bar and the spiral arms but yield interesting results for the nuclear region.
Joersaeter Steven
Lindblad Per Olof
Sandqvist Aa
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