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

Short time scale variability of the BL Lacertae object OJ 287 in the near-infrared

Journal Article · · Astrophysical Journal, Supplement Series; (USA)
DOI:https://doi.org/10.1086/191370· OSTI ID:7266019
; ; ;  [1]
  1. CNR, Istituto di Fisica dello Spazio Interplanetario, Frascati (Italy) Roma I Universita, Rome (Italy)
The results of a NIR photometric monitoring of the BL Lac object OJ 287 are presented. The standard JHK photometry shows variability of maximum amplitude of about 0.7 mag over the entire observing period of 23 months and about 0.3 mag on time intervals as short as about 3 hr. No spectral variability has been found. A fast monitoring performed in the H band, with a sampling period of about 4 min, provides evidence that variations can occur in this object on time scales of over 4 min and with an rms amplitude of 6-7 percent. These variations show slow increasing and fast decreasing trends, but no clear indication of periodicity is apparent. 30 refs.
OSTI ID:
7266019
Journal Information:
Astrophysical Journal, Supplement Series; (USA), Journal Name: Astrophysical Journal, Supplement Series; (USA) Vol. 71; ISSN APJSA; ISSN 0067-0049
Country of Publication:
United States
Language:
English

Similar Records

COLOR BEHAVIOR OF BL LACERTAE OBJECT OJ 287 DURING AN OPTICAL OUTBURST
Journal Article · Mon Feb 14 23:00:00 EST 2011 · Astronomical Journal (New York, N.Y. Online) · OSTI ID:21583227

BL Lacertae objects: The case for synchronous optical-radio outbursts in OJ 287
Journal Article · Sat Sep 01 00:00:00 EDT 1979 · Astron. J.; (United States) · OSTI ID:5929697

Optical variability of two X-ray-selected and nine radio-selected BL Lac objects
Journal Article · Fri Jul 01 00:00:00 EDT 1988 · Astron. J.; (United States) · OSTI ID:6766824