Universitat de Barcelona
2026-03-19T10:56:01Z
2026-03-19T10:56:01Z
2006-01
2026-03-19T10:56:01Z
The status of the Calar Alto Lunar Occultation Program is presented. This has been conducted at IR and optical wavelengths through OAN 1.5-m and CAHA 2.2-m telescopes, operating either with fast IR array or CCD. The scientific throughput is double: first, angular diameter determinations (>1-2 mas) of late-type stars and circumstellar matter detection of astrophysically interesting targets (YSOs, T Taus, carbon stars, masers). Second, new binaries detection with projected separations > 5mas, and brightness ratios up to 1:50. We detail the runs carried out so far and summarize the scientific results obtained.
Article
Versió publicada
Anglès
Satèl·lits científics; Observatoris astronòmics; Geologia lunar; Scientific satellites; Astronomical observatories; Lunar geology
Instituto de Astronomía, Universidad Nacional Autónoma de México
Reproducció del document publicat a: https://astronomia.unam.mx/journals/rmxac/article/view/2006rmxac..25..101f
Revista Mexicana de Astronomia y Astrofisica, 2006, vol. 25, p. 101-102
https://astronomia.unam.mx/journals/rmxac/article/view/2006rmxac..25..101f
(c) Instituto de Astronomía, Universidad Nacional Autónoma de México, 2006
