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- W2183627711 abstract "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 (mV 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." @default.
- W2183627711 created "2016-06-24" @default.
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- W2183627711 date "2002-01-01" @default.
- W2183627711 modified "2023-09-26" @default.
- W2183627711 title "THE LBV PHASE OF THE PLANETARY NEBULA LMC-N66 1" @default.
- W2183627711 hasPublicationYear "2002" @default.
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