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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...

Whakaahuatanga katoa

I tiakina i:
Ngā taipitopito rārangi puna kōrero
I whakaputaina i:Revista Mexicana de Astronomía y Astrofísica
Kaituhi matua: F. Millour
Hōputu: Artigo
Reo:Espanhol
I whakaputaina: Universidad Nacional Autónoma de México 2010
Ngā marau:
Urunga tuihono:https://www.redalyc.org/articulo.oa?id=57115706002
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