Spectroscopic versus photometric metallicities: Milky Way dwarf spheroidal companions as a test case

Astronomy and Astrophysics

Volumn 531, Issue , 2011, Pages

  Lianou, S ^a   Grebel, E K ^a   Koch, A ^b,c  

^a ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c UNIVERSITÄT HEIDELBERG   (Germany)

Author keywords

Galaxies: abundances; Galaxies: dwarf; Galaxies: stellar content; Local Group

Indexed keywords

GALAXIES: ABUNDANCES; GALAXIES: DWARF; GALAXIES: STELLAR CONTENT; HIGH-RESOLUTION SPECTRA; ISOCHRONES; LOCAL GROUPS; LOW RESOLUTION; METALLICITIES; MILKY WAYS; NEAR INFRARED; PHOTOMETRIC DATA; PHOTOMETRIC METHOD; RED GIANT BRANCHES; SPECTRAL SYNTHESIS; STELLAR POPULATIONS; TEST CASE;

ASTROPHYSICS; CALCIUM; DISTRIBUTION FUNCTIONS; GALAXIES; HARMONIC ANALYSIS; SPECTROSCOPIC ANALYSIS; SPECTROSCOPY; STARS;

PHOTOMETRY;

EID: 79959941680     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116998     Document Type: Article

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