NGC 2108 stellar cluster in the LMC

NGC 2108 is a rich "mid-aged" cluster, about 600 million years old. A careful comparison with its neighbour NGC 2093 shows that the brightest stars of NGC 2108 are fainter and whiter than the brightest members of NGC 2093; this indicates that NGC 2108 is older. Note also the distinctly red star to the East (left) of the center of this cluster. This is a member of a stellar class referred to as "Carbon stars", cool giant stars that are characterized by the presence of carbon molecules (C2) in their atmospheres and having extremely red colours. This sky field measures 2.8 x 2.6 arcsec. North is up and East is left.

Kilde:

ESO

Om billedet

Id:eso0437h
Type:Observation
Udgivelsesdato:10. december 2004
Relaterede pressemeddelelser:eso0437
Størrelse:702 x 668 px

Om objektet

Navn:NGC 2108
Type:Local Universe : Star : Grouping : Cluster
Afstand:170000 lysår
Constellation:Dorado
Kategori:Star Clusters

Billedformater

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Koordinater

Position (RA):5 44 26.57
Position (Dec):-69° 8' 47.11"
Field of view:2.81 x 2.67 arcminutes
Orientering:Nord er 0.5° venstre fra lodret

Farver & filtre

BåndTeleskop
Ultraviolet
U
MPG/ESO 2.2-metre telescope
WFI
Optisk
Oiii
MPG/ESO 2.2-metre telescope
WFI
Optisk
H-alpha
MPG/ESO 2.2-metre telescope
WFI