AG Dra

The third object to be studied under the multi-wavelength monitoring program was the symbiotic system AG Draconis. A summary of the observations that have been performed so far during the outburst, plus UBVR light curves from the Katzman Automatic Imaging Telescope (KAIT) can be seen below.

The red arrows indicate when observations with the X-Ray Multi-Mirror Satellite (XMM), the Very Large Array (VLA), and optical spectroscopy were performed.

The KAIT UBVR light curves are differential, and so except for the V-band light curve, which has been shifted to match the early light curve from the American Association of Variable Star Observers (green diamonds), the magnitude scale is arbitrary.


Last modified: Mon Oct 27 11:55:58 EST 2003