Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-05-14
Astronomy and Astrophysics
Astrophysics
6 pages text, 3 figures, accepted in ApJ Letters
Scientific paper
This is the first report on the new outburst presented by the central star of the LMC-N66 nebula. This object was classified as a planetary nebula, however, its true nature is under debate. In the period 1955-1990 the central star was almost undetectable and only nebular emission lines were observed. In 1990, the beginning of an outburst was detected and in few months it became much brighter and developed wide He and N lines, typical of a Wolf Rayet star of the N-sequence. The maximum occurred in 1994 and afterwards the star slowly faded. Analysis of its evolution showed that it has a variable mass-loss rate which occasionally increases enormously, creating a false photosphere at a much larger radius, making it appear a few magnitudes brighter. The present outburst has occurred 13 years after the episode from 1994 to 2000. So far this new event has similar characteristics although there are some significant differences in the spectral features. We present optical and FUSE spectra showing the main properties of this latter event.
Hamann Wolf-Rainer
Pena Miriam
Rojo Patricio
Ruiz María Teresa
Torres-Peimbert Silvia
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