Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...403...93n&link_type=abstract
Astronomy and Astrophysics, v.403, p.93-103 (2003)
Astronomy and Astrophysics
Astrophysics
30
Stars: Agb And Post-Agb, Stars: Carbon, Galaxies: Local Group, Galaxies: Individual: Ngc 185, Ngc 147, Surveys
Scientific paper
We present results of our ongoing photometric survey of Local Group galaxies, using a four filter technique based on the method of Wing (\cite{Wing71}) to identify and characterise the late-type stellar content. Two narrow band filters centred on spectral features of TiO and CN allow us to distinguish between AGB stars of different chemistries [M-type (O-rich) and C-type (C-rich)]. The major parts of two dwarf galaxies of the M 31 subgroup - NGC 185 and NGC 147 - were observed. From photometry in V and i we estimate the tip of the RGB, and derive distance moduli respectively. With additional photometric data in the narrow band filters TiO and CN we identify 154 new AGB carbon stars in NGC 185 and 146 in NGC 147. C/M ratios are derived, as well as mean absolute magnitudes
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 form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strabg.fr/cgi-bin/qcat?J/A+A/403/93
Kerschbaum Florian
Nowotny Walter
Olofsson Hans
Schwarz Hugo E.
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