ON DETERMINATION OF ANGULAR SIZES OF SOME RELATIVELY HOT STARS BY LUNAR OCCULTATION OBSERVATIONS AND ON SUGGESTED INTERFEROMETRIC INVESTIGATION OF THESE STAR
Interferometric and lunar occultation observations of stars are both the e ective techniques which allow us toreach high angular resolution at a level of 1 milliarcsecond and better both in the visual and in the near-IRspectral ranges. Several tens of photoelectric di raction curves of the lunar occ...
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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autor: | |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2010
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57115706047 |
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