Flare at OIR wavelengths in GX 339-4

Details Flare at OIR wavelengths in GX 339-4 Flare at OIR wavelengths in GX 339-4

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1109....1b&link_type=abstract

The Astronomer's Telegram, #1109

Astronomy and Astrophysics

Astronomy

3

Infra-Red, Optical, Binaries, Black Holes, Transients

Scientific paper

We have continued our observations of GX 339-4 with the SMARTS 1.3m and
ANDICAM instrument since the source transitioned into the hard state
around MJD 54233 (13th May 2007, ATEL #1074). The optical and infrared
(OIR) fluxes reached a minimum at MJD 54239, and then began to rise.
Since that time the brightness of the source has increased as follows.

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