Kinematic mapping of the high-excitation gas in NGC 1365

Details Kinematic mapping of the high-excitation gas in NGC 1365 Kinematic mapping of the high-excitation gas in NGC 1365

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234..155e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Sept. 1, 1988, p. 155-158.

Other

16

Cosmic Gases, Gas Dynamics, Oxygen Spectra, Spiral Galaxies, Astronomical Maps, Fabry-Perot Interferometers, H Alpha Line, Velocity Distribution

Scientific paper

The authors present TAURUS data on the [O III], λ5007
line-emission from the nuclear regions of the active barred spiral
galaxy NGC 1365. The velocity map clearly confirms the existence of line
splitting and allows to identify one component with the disc, while the
other components appear to be best interpreted as bipolar outflow.

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