Multiwavelength observations of the February 1996 high-energy flare in the blazar 3C 279

Details Multiwavelength observations of the February 1996 high-energy flare in the blazar 3C 279 Multiwavelength observations of the February 1996 high-energy flare in the blazar 3C 279

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1417w&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1417-1422 (1997).

Astronomy and Astrophysics

Astronomy

Active And Peculiar Galaxies And Related Systems, Magnitudes And Colors, Luminosities, Gamma-Ray Sources, Gamma-Ray Bursts, Astronomical Observations

Scientific paper

We report CGRO, RXTE, ASCA, ROSAT, IUE, HST and ground-based observations of a large flare in 3C 279 in February 1996. X-rays and γ-rays peaked simultaneously (within one day). We show simultaneous spectral energy distributions prior to and near the flare peak. The γ-ray flare was the brightest ever observed in this source.

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