SIMBAD references

2011MNRAS.414.3492M - Mon. Not. R. Astron. Soc., 414, 3492-3500 (2011/July-2)

Asymptotic giant branch stars in the Sculptor dwarf spheroidal galaxy.

MENZIES J.W., FEAST M.W., WHITELOCK P.A. and MATSUNAGA N.

Abstract (from CDS):

JHKS photometry is presented for a 35 arcmin2 field centred on the Sculptor dwarf spheroidal galaxy. With the aid of published kinematic data definite galaxy members are identified and the width in J-K of the colour–magnitude diagram is shown to be consistent with an old population of stars with a large range in metal abundance. We identify two Asymptotic Giant Branch variables, both carbon Miras, with periods of 189 and 554 d, respectively, and discuss their ages, metallicities and mass-loss as well as their positions in the Mira period–luminosity diagram. There is evidence for a general period–age relation for Local Group Miras. The mass-loss rate for the 554-d variable, MAG29, appears to be consistent with that found for Miras of comparable period in other Local Group galaxies.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

Journal keyword(s): stars: AGB and post-AGB - stars: carbon - galaxies: individual: Sculptor-Local Group - galaxies: stellar content

VizieR on-line data: <Available at CDS (J/MNRAS/414/3492): table2.dat>

Nomenclature: Table 2: [MFW2011] NNNNN N=1797 among (Nos 1001-27026).

Simbad objects: 1793

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2020.02.29-05:18:34

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