Optical monitoring of HD 106225.

Details Optical monitoring of HD 106225. Optical monitoring of HD 106225.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...302..407h&link_type=abstract

Astronomy and Astrophysics, v.302, p.407

Astronomy and Astrophysics

Astrophysics

1

Gamma Rays: Bursts: Stars: Hd 106225

Scientific paper

The RS CVn system HD 106225 has been suggested recently as the possible optical counterpart of the luminous gamma ray burst GRB 930103. We report here on the results of an analysis of the object on Ondrejov sky patrol plates. The star does not exhibit light variations exceeding mag 0.3 within a monitoring interval of 180h and exceeding mag 0.8 within a monitoring interval of 420h.

Affiliated with

Also associated with

No associations

Rating

Optical monitoring of HD 106225. 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 Optical monitoring of HD 106225., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical monitoring of HD 106225. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1351227