Carbon-rich stars (C stars) of Population II, such as CH giants, can provide direct information on the role of low-to-intermediate-mass stars of the Halo in early Galactic evolution. Moreover, accurate knowledge of the CH stellar population is a critical requirement for building up scenarios for early Galactic chemical evolution.
New bright carbon stars found in the DFBS / K. S., Gigoyan; Rossi, Corinne; Sclavi, Silvia; Gaudenzi, Silvia. - In: ASTROPHYSICS. - ISSN 0571-7256. - STAMPA. - 55:3(2012), pp. 424-428. [10.1007/s10511-012-9248-3]
New bright carbon stars found in the DFBS
ROSSI, Corinne;SCLAVI, SILVIA;GAUDENZI, Silvia
2012
Abstract
Carbon-rich stars (C stars) of Population II, such as CH giants, can provide direct information on the role of low-to-intermediate-mass stars of the Halo in early Galactic evolution. Moreover, accurate knowledge of the CH stellar population is a critical requirement for building up scenarios for early Galactic chemical evolution.File allegati a questo prodotto
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