SIMBAD references

2013MNRAS.433.1966O - Mon. Not. R. Astron. Soc., 433, 1966-1969 (2013/August-2)

Segue 3: the youngest globular cluster in the outer halo.

ORTOLANI S., BICA E. and BARBUY B.

Abstract (from CDS):

Deep Galileo (Telescopio Nazionale Galileo) B, V and I images of Segue 3, reaching V ∼ 25, reveal that it is the youngest globular cluster known so far in the Galaxy. A young age of 3.2Gyr is found, differently from a previous estimate of 12Gyr. It also appears to be moderately metal rich with [Fe/H] ∼ -0.8, rather than [Fe/H] ∼ -1.7, as previously suggested by Fadely et al. A main difference in the age derivation relative to Fadely et al. comes from the consideration of subgiant branch stars in the isochrone fitting. A deduced distance of d☉ = 29.1kpc is compatible with the outer halo location of other low luminosity globular clusters.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): Hertzsprung-Russell and colour-magnitude diagrams - globular clusters: individual: Segue 3 - Galaxy: halo

VizieR on-line data: <Available at CDS (J/MNRAS/433/1966): seg3viac.dat seg3vibc.dat>

Nomenclature: seg3viac.dat: [OBB2013] NNNN N=1103 among (Nos 1-1248).

Status at CDS:   will not be processed
// All or part of tables of objects will not be ingested in SIMBAD.

Simbad objects: 12

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2020.06.01-08:48:55

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