A new analysis of the 11-year period in OJ287 - Confirmation of its existence

Details A new analysis of the 11-year period in OJ287 - Confirmation of its existence A new analysis of the 11-year period in OJ287 - Confirmation of its existence

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...264...32k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 264, no. 1, p. 32-36.

Astronomy and Astrophysics

Astronomy

70

Bl Lacertae Objects, Black Holes (Astronomy), Accretion Disks, Light Curve

Scientific paper

We have compiled all the available optical B band data on OJ287, between 1890 and 1991. Using this data we have found a period of 11.6 +/- 0.5 yr for the outbursts in OJ 287. This value is in good agreement with the period of 11.65 yr between outbursts and 11.05 yr between minima found previously by Sillanpaa et al. (1988), using V-band data. Based on this period we can predict that the next outburst should be at its maximum around August 1994.

Affiliated with

Also associated with

No associations

Rating

A new analysis of the 11-year period in OJ287 - Confirmation of its existence does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A new analysis of the 11-year period in OJ287 - Confirmation of its existence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A new analysis of the 11-year period in OJ287 - Confirmation of its existence will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1868056