Fairall 9
Right ascension: 1:21:51.2 Magnitude: 13.2
Declination: -59:03:59
Image: SWP 14157
Date: 1981 Jun 2 6:26 UT
Exposure duration: 30 min x 3 exposures offset in large aperture
Fairall 9 shows a typical Seyfert galaxy spectrum: a strong non-stellar
continuum with broad emission lines (Lyman alpha, N V, Si IV, and C IV) are
present). The continuum is likely produced by a very hot accretion disk
surrounding a postulated supermassive black hole (about 100 million solar
masses) near the galaxy's center. The emission lines are also produced
in the accretion disk, and are broadened by rotational Doppler effects as
the gas moves around the central continuum source. The width of the
lines suggests velocities as high as ten percent of the speed of light,
supporting the model of an extremely massive but compact central object
around which the gas moves.
Last updated: 08 April 1998
Obtained from IUE project at Goddard Space Flight Center