Sorveglianza spettroscopica di stelle variabili luminose

Details Sorveglianza spettroscopica di stelle variabili luminose Sorveglianza spettroscopica di stelle variabili luminose

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asuai...2...65d&link_type=abstract

Astronomia. La rivista dell'Unione Astrofili Italiani (ISSN 0392-2308), N. 2, p. 65 - 68 (marzo-aprile 2003)

Other

Variables: Spectra

Scientific paper

With a spectrograph fitted with an MOS Linear Image Sensor resolving 12 nm/mm at Hγ, we systematically study γ Cas, β Lyr and α Ori between 400 and 1000 nm. γ Cas reveals Hβ and Hα bands in emission and telluric O2 and H2O bands. The spectra show also weak absorptions near 610, 771, 776 and 781 nm, which appear to vary in intensity, and another one at 630 nm which remains constant.

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