The age of the old Magellanic Cloud clusters - II. NGC 1786, 1841 and 2210 as evidence for an old coeval population of LMC and galactic globular clusters

Monthly Notices of the Royal Astronomical Society

Volumn 282, Issue 2, 1996, Pages 614-622

  Brocato, E ^a   Castellani, V ^a,b   Ferraro, F R ^c   Piersimoni, A M ^a   Testa, V ^d,e  

^a INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^b UNIVERSITY OF PISA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^d UNIVERSITY OF BOLOGNA   (Italy)

^e MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Galaxies: evolution; Galaxies: star clusters; Globular clusters: general; Magellanic clouds

Indexed keywords

ASTROPHYSICS; GALAXIES; UNCERTAINTY ANALYSIS;

CLOUD CLUSTERS; COLOR-MAGNITUDE DIAGRAMS; COLOUR-MAGNITUDE DIAGRAMS; GALAXIES: STAR CLUSTERS; GALAXY EVOLUTION; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; LARGE MAGELLANIC CLOUDS; MAGELLANIC CLOUDS; UNCERTAINTY;

METALS;

EID: 0041137979     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/282.2.614     Document Type: Article

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