Integrated J-and H-band spectra of globular clusters in the LMC: Implications for stellar population models and galaxy age dating

Astronomy and Astrophysics

Volumn 543, Issue , 2012, Pages

  Lyubenova, M ^a   Kuntschner, H ^b   Rejkuba, M ^b   Silva, D R ^c   Kissler Patig, M ^b   Tacconi Garman, L E ^b  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

Author keywords

Galaxies: star clusters: general; Magellanic Clouds; Stars: carbon

Indexed keywords

AGE DATING; ASYMPTOTIC GIANT BRANCH STARS; CARBON STARS; CARBON-BASED; EMPIRICAL CALIBRATION; FEATURE STRENGTH; GALAXIES: STAR CLUSTERS; GLOBULAR CLUSTERS; INTEGRAL FIELD SPECTROGRAPH; LARGE MAGELLANIC CLOUDS; MAGELLANIC CLOUDS; METALLICITIES; MODEL PREDICTION; NEAR-IR; OLDER POPULATION; PILOT PROJECTS; RED GIANT BRANCHES; SPECTRAL ENERGY DISTRIBUTION; SPECTRAL LIBRARIES; SPECTRAL RANGE; SPECTRAL SHAPES; STAR CLUSTERS; STARS: CARBON; STELLAR POPULATIONS; WAVELENGTH RANGES; WAVELENGTH REGIMES; WEALTH OF INFORMATION;

C (PROGRAMMING LANGUAGE); CALIBRATION; CARBON; GALAXIES; INTEGRATION; MATHEMATICAL MODELS;

STARS;

EID: 84863227908     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201218847     Document Type: Article

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