HOT STARS AND INTERFEROMETRY
What is long-baseline optical/IR stellar interferometry? A few years ago, many astronomers might not have been able to answer that question properly. This is today hopefully not the case anymore, because mainstream facilities, such as the VLTI, the Keck-I or the CHARA array, o er now this delicate t...
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| 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: | Espanhol |
| 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=57115706002 |
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