Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Spectropolarimetry of Cygnus A and the scattering model for the extended continuum

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/185569· OSTI ID:7163861
;  [1]
  1. Lick Observatory, Santa Cruz, CA (USA)
Previous work on the peculiar double radio galaxy Cyg A has shown that the blue optical continuum in this object is extended over a region about 3 kpc in size. Spectropolarimetry of Cyg A is presented in order to test the hypothesis that this extended continuum source represents light scattered from an otherwise hidden active nucleus. The observed continuum polarization of 1.58 percent at position angle 13 deg is quite low, probably indicating that an explanation in terms of scattering is untenable. Instead, it is proposed that the blue continuum seen in the optical is light from hot stars, essentially unrelated to the active nucleus. The nucleus itself is still presumed to be hidden from direct view, either by an intervening dust lane or by an obscuring torus surrounding the nucleus. 14 refs.
OSTI ID:
7163861
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 346; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

The galaxy continuum in the spectrum of Cygnus A
Journal Article · Fri Dec 31 23:00:00 EST 1982 · Publ. Astron. Soc. Pac.; (United States) · OSTI ID:5683312

Subaru spectroscopy and spectral modeling of Cygnus A
Journal Article · Tue Jun 10 00:00:00 EDT 2014 · Astrophysical Journal · OSTI ID:22356725

Spectropolarimetry of 3CR 68.1: A Highly Inclined Quasar
Journal Article · Wed Jul 01 00:00:00 EDT 1998 · Astrophysical Journal · OSTI ID:664874