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Paper detail

AGB stars and the plate archives heritage

We report on the characterization of a number of AGB candidate stars identified with objective-prism plates of the Byurakan Observatory. Digitized photographic sky survey plates and recent CCD photometry have been used to improve the selection and distinguish variable and non-variable stars. Some comparisons among published catalog magnitudes are also made. Slit spectroscopy from the Asiago and Loiano Observatories allowed a firm spectral classification, separating C-Type, N-Type and normal M giants. Color-color plots using WISE, AKARI and 2MASS J-band data allow an efficient discrimination of spectral types, which can be used for the definition of larger statistical samples.

preprint2014arXivOpen access
Roberto NesciSilvia GaudenziCorinne RossiCamilla PezzottiKamo GigoyanNicolas Mauron
astro-ph.SR
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Roberto NesciSilvia GaudenziCorinne RossiCamilla PezzottiKamo GigoyanNicolas Mauron

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