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...
Na minha lista:
| 發表在: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| 主要作者: | |
| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
Universidad Nacional Autónoma de México
2002
|
| 主題: | |
| 在線閱讀: | https://www.redalyc.org/articulo.oa?id=57112050 |
| 標簽: |
沒有標簽, 成為第一個標記此記錄!
|