Using spectroscopic data to disentangle stellar population properties

Astronomy and Astrophysics

Volumn 409, Issue 2, 2003, Pages 511-522

  Cardiel, N ^a,b   Gorgas, J ^b   Sanchez Blazquez P ^b   Cenarro, A J ^b   Pedraz, S ^a,b   Bruzual, G ^c   Klement, J ^d  

^a CENTRO ASTRONÓMICO HISPANO ALEMÁN   (Spain)

^b UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

^c CENTRO DE INVESTIGACIONES DE ASTRONOMÍA   (Venezuela)

^d ETH ZURICH   (Switzerland)

Author keywords

Galaxies: stellar content; Methods: data analysis; Techniques: spectroscopic

Indexed keywords

LUMINESCENCE; OPTICAL TELESCOPES; PLANETS; SOLAR RADIATION;

STELLAR CONTENT;

GALAXIES;

EID: 0141958788     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031096     Document Type: Article

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