On the difference between nuclear and contraction ages

Astronomy and Astrophysics

Volumn 453, Issue 1, 2006, Pages 101-119

  Lyra, W ^a,b,c   Moitinho, A ^d   Van Der Bliek, N S ^a   Alves, J ^e  

^a CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^b FEDERAL UNIVERSITY OF RIO DE JANEIRO   (Brazil)

^c BOX 515   (Sweden)

^d UNIVERSITY OF LISBON   (Portugal)

^e EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Galaxies: star clusters; Galaxy: open clusters and associations: general; Hertzsprung Russell (HR) and C M diagrams; Stars: formation; Techniques: photometric

Indexed keywords

COLOR IMAGE PROCESSING; GALAXIES; GRAPH THEORY; MATHEMATICAL MODELS; NUMERICAL ANALYSIS; PHOTOMETRY; STATISTICAL TESTS; TEMPERATURE CONTROL;

GALAXIES: STAR CLUSTERS; GALAXY: OPEN CLUSTERS AND ASSOCIATIONS; HERTZSPRUNG-RUSSELL (HR) AND C-M DIAGRAM; STAR: FORMATION; TECHNIQUES: PHOTOMETRIC;

ASTROPHYSICS;

EID: 33745757363     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053894     Document Type: Article

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