Physics – Optics
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...410..552a&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 410, no. 2, p. 552-566.
Physics
Optics
22
Active Galactic Nuclei, Fiber Optics, Spiral Galaxies, Astronomical Spectroscopy, Emission Spectra, Optical Fibers, Red Shift, Seyfert Galaxies, Spectral Line Width
Scientific paper
A 2D array of optical fibers generating simultaneous spectral and spatial information has been used to observe the central 13 arcsec of NGC 5728; on this basis, an analysis of the morphology and kinematics of the galaxy's circumstellar environment is conducted. The kinematic center coincides with the peak in radio emission, but is separated by about 1 arcsec from the maxima of the H-alpha and forbidden N II and S II emission. This strongly suggests that the active nucleus is obscured, and explains the nuclear redshift as well as the high ratio of circumnuclear-to-nuclear flux emission previously reported.
Arribas Santiago
Mediavilla Evencio
No associations
LandOfFree
The circumstellar region of NGC 5728 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The circumstellar region of NGC 5728, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The circumstellar region of NGC 5728 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1735546