The rapid fading of V1647 Orionis: the sudden end of a FUor-type eruption?
The young eruptive star V1647 Ori started a rapid fading in October 2005 and now is only 1 mag above the pre-outburst level. Colour changes indicate that the fading is not due to increasing extinction.
Kospal, Agnes et al.
Fecha de publicación:
11
2005