Published April 15, 1979 | Version v1
Journal article

Quasars aligned across NGC 3384

  • 1. Hale Observatories, Carnegie Institution of Washington, California Institute of Technology

Description

A number of ultraviolet-excess stellar objects were found in the vicinity of the triple system of galaxies NGC 3379/84/89. Systematic search of an area with radius 30' (0.77 deg2) around these galaxies yields eight quasars aligned across NGC 3384. Six of these quasars appear to have very similar redshifts, between z=1.11 and z=1.28. The two quasars closest to NGC 3384 are aligned exactly across its high-surface-brightness nucleus and have redshifts z=1.107 and z=1.111. Ultraviolet-excess objects have been cataloged by G. d. T. on the entire 10 inch x 10 inch (25.4 cm x 25.4 cm) Palomar Schmidt plate on which the original NGC 3384 association was seen. The total area is 20.9 deg2, and 422 ultraviolet objects were found. All candidates in the 0.77 deg2 field were observed spectroscopically; when the numbers of stars and quasars found there wereextrapolated to the whole plate, a quasar density of 7 +- 4 deg-2 down to B=20 mag was derived. This value agrees well with the Sandage and Luyten value of 10 and the Setti and Woltjer value of 8.5 deg-2 to the same magnitude limit

Additional details

Publishing Information

Journal Title
Astrophys. J.
Journal Volume
229
Journal Issue
2
Series
Astrophys. J.
Journal Page Range
489-495
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
10489406
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ALIGNMENT; ENERGY SPECTRA; GALAXIES; GALAXY CLUSTERS; QUASARS; RED SHIFT; SPECTROSCOPY; ULTRAVIOLET RADIATION
Descriptors DEC
COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; RADIATIONS; SPECTRA