Other
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...309...45k&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 309, Oct. 1, 1986, p. 45-58.
Other
23
Astronomical Photometry, Infrared Photometry, Radio Galaxies, Stellar Rotation, X Ray Sources, Astronomical Spectroscopy, Galactic Nuclei, Heao 2, Mass To Light Ratios, Stellar Color, X Ray Imagery
Scientific paper
The authors present stellar rotation and velocity dispersion data, optical surface photometry, Einstein Observatory IPC X-ray data, and aperture (optical and infrared) photometry of the radio galaxy IC 4296. It is found that the projected stellar rotation axis is misaligned with the projected radio axis by ≡28°. The photometric major and minor axis surface brightness profiles of IC 4296 are well represented by King (1966) models in the range 3arcsec < r < 100arcsec. The central mass-to-light ratio is M/LB = (13±3)h (h Hubble constant in units of 100 km s-1Mpc-1). The IPC X-ray image shows a slightly resolved source centered on IC 4296. Isothermal, hydrostatic atmospheres that are consistent with the X-ray data can be constructed.
Bicknell Geoffrey V.
Carter David
Killeen Neil E. B.
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