The LBV Phase of the Planetary Nebula LMC-N66

Details The LBV Phase of the Planetary Nebula LMC-N66 The LBV Phase of the Planetary Nebula LMC-N66

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12..148p&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

1

Planetary Nebulae: Individual (Lmc-N66), Stars: Wolf-Rayet

Scientific paper

Recent observations of the [WN] central star of the planetary nebula LMC-N66, combined with previous data show that the star has been slowly fading, after its violent LBV-type outburst occurred in 1994. The present stellar brightness ( m[V] ~ 18.1 mag) and the probable mass loss rate are similar to the values observed in 1990. Nebular data from long-slit STIS-HST observations allow us to analyze some nebular characteristics.

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