(the following information provided by Dr. Pierre Chayer)
Drs. Jeremy Drake (Harvard-Smithsonian Center for Astrophysics), Robert Stern (Solar and Astrophysics Laboratory, Lockheed Martin), Guy Stringfellow (University of Colorado), Mihalis Mathioudakis (Armagh Observatory, Northern Ireland), Martin Laming (E. O. Hulburt Center for Space Research), and David Lambert (University of Texas at Austin) reported the detection of quiescent EUV emission from the very low mass dwarf star VB 8 by the Extreme Ultraviolet Explorer (EUVE) in the Lexan/B band (65-190 Angstrom). The observation of VB 8 spanned the period 1994 July 30 23:08 to 1994 August 8 23:59 with an effective exposure time of about 200 ks. This observation allowed the detection of VB 8 as a source in the resulting EUVE Deep Survey detector image, with a count rate of 1.98 count ks-1. Dr. Drake and his collaborators interpret this emission in terms of a hot coronal plasma. Combining observations made by Einstein (X-ray satellite), ROSAT (Rontgen Satellite), and EUVE between 1979 and 1994, they argue that their results are consistent with the picture of a turbulently driven or distributive dynamo for VB 8, rather than with a large-scale field dynamo which appears dominate the solar corona. For further information about this report, you may refer to the original article published in The Astrophysical Journal, Vol. 469, page 828.
Drs. Knox Long (Space Telescope Science Institute), Christopher Mauche (Lawrence Livermore National Laboratory), John Raymond (Harvard-Smithsonian Center for Astrophysics), Paula Skody (University of Washington), and Janet Mattei (American Association of Variable Star Observers) reported the observation of U Geminorum during the peak and declining phases of a wide outburst with the Extreme Ultraviolet Explorer (EUVE) satellite. Known as one of the brightest dwarf nova at outburst, U Geminorum was one of the brightest EUV sources in the sky at its maximum. The observations of U Geminorum were carried out with the spectrometers on EUVE, beginning on December 28 and extending through 1994 January 8. For further information about this report, you may refer to the original article published in The Astrophysical Journal, Vol. 469, page 841.
See attached PostScript Figure