THE NATURE OF STARS WITH THE B[E] PHENOMENON THROUGH INTERFEROMETRIC EYES
The recently dened Galactic FSCMa group comprises -40 not very luminous objects that signicantly expand the luminosity range of hot dust-forming stars. These objects exhibit extremely strong emission-line spectra and IR excesses, which are indicative of compact dust envelopes. They are most likely b...
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 第一著者: | |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2010
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57115706036 |
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