Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...427..613k&link_type=abstract
Astronomy and Astrophysics, v.427, p.613-619 (2004)
Astronomy and Astrophysics
Astrophysics
11
Stars: Agb And Post-Agb, Stars: Carbon, Galaxies: Local Group, Galaxies: Individual: And Ii, Techniques: Photometric, Surveys
Scientific paper
Our photometric survey of Local Group galaxies, using a four filter technique based on the method of Wing (\cite{Wing71}) allows the identification and subsequent characterization of their late-type stellar content. Two narrow band filters centred on molecular bands of TiO and CN allow us to distinguish between AGB stars of different chemistries [M-type (O-rich) and C-type (C-rich)]. The faint dwarf spheroidal galaxy And II, a member of the M 31 subgroup, was surveyed. From photometry in V and i as well as in the narrow band filters TiO and CN we were able to identify 7 new AGB carbon stars, to derive their mean absolute
Based on observations made with the Nordic Optical Telescope operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias.
Table A.1. is only available in electronic at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/427/613}}
Kerschbaum Florian
Nowotny Walter
Olofsson Hans
Schwarz Hugo E.
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