The lbv phase of the planetary nebula lmc-n66
Recent observations of the [WN] central star of the planetary nebula LMC-N66, combined with previous datashow that the star has been slowly fading, after its violent LBV-type outburst occurred in 1994. The presentstellar brightness (mV 18:1 mag) and the probable mass loss rate are similar to the va...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2002
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57112050 |
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