Variable Stars - NQ Vul
Type Slow Novae Click for lightcurve Slow novae that fade after maximum light by 3 magnitudes in ≥ 150 days. Here the presence of the well-known "dip" in the light curves of novae similar to T Aur and DQ Her is not taken into account: The rate of fading is estimated on the basis of a smooth curve, its parts before and after the "dip" being a direct continuation of one another. AAVSO Legacy Cataclysmic Variable Programme
Hills Observatory: 1 January 2013 to 15 December 2018
COMETS COMETS
DEEP SKY DEEP SKY