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

Imaging spectroscopy of five QSOs

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/164898· OSTI ID:6581510
Direct images and spatially resolved spectra have been obtained for five QSOs having a wide range of radio, optical, and X-ray luminosity. The two lowest luminosity objects clearly show absorption features identified with stars in a host galaxy at the QSO redshift. Such features are possibly seen in two others but not in the highest luminosity object, in which nebulosity is barely discernable. All objects show off-nuclear changes in continuum color and in emission-line intensities and ratios. The radio-loud objects have more luminous host galaxies, strong and extended forbidden O II and forbidden O III, and UV-bright nuclei. They tend to have optically luminous nuclei, high nuclear to galaxy luminosity ratios, and blue host galaxies. 23 references.
Research Organization:
British Columbia Univ., Vancouver; Dominion Astrophysical Observatory, Victoria
OSTI ID:
6581510
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 312; ISSN ASJOA
Country of Publication:
United States
Language:
English

Similar Records

Nature of QSO host galaxies
Journal Article · Tue Jul 01 00:00:00 EDT 1986 · Astrophys. J.; (United States) · OSTI ID:7262306

What is the difference between radio-loud and radio-quiet quasi-stellar objects
Journal Article · Sat Jul 01 00:00:00 EDT 1989 · Astrophysical Journal; (USA) · OSTI ID:5509900

Radio-loud and radio-quiet QSOs
Journal Article · Wed Nov 09 23:00:00 EST 2016 · Astrophysical Journal · OSTI ID:22869211