2MASS J19210666+3743033 , the SIMBAD biblio

2009MNRAS.393..272W - Mon. Not. R. Astron. Soc., 393, 272-296 (2009/February-2)

Metallicities and radial velocities of five open clusters including a new candidate member of the Monoceros stream.

WARREN S.R. and COLE A.A.

Abstract (from CDS):

Near-infrared spectra of 133 red giant stars from 10 Galactic open clusters and two Galactic globular clusters spanning 2.2dex in metallicity and 11Gyr in age are presented. We combine this sample with 10 clusters from Cole and collaborators to investigate the Caii triplet line strengths and their relation to cluster metallicity and position along the red giant branch. We show that characterizing the stellar surface gravity using Ks-band photometry (relative to the horizontal branch) taken from the Two Micron All-Sky Survey allows for metallicity measurements at least as precise as those derived using V- or I-band data. This has the great advantage that uniform photometry and reliable astrometry are available for a large number of clusters. Using Ks-band photometry also reduces the effect of differential reddening within a given cluster. We find no significant evidence for age or metallicity effects to the linear Caii triplet-metallicity relationship over the small range in magnitudes studied when homogeneous reference metallicities are used. We derive the first spectroscopic metallicity and new radial velocity estimates for five open clusters: Berkeley81, Berkeley99, IC1311, King2 and NGC7044. King2 has an anomalous radial velocity compared with the local disc population. We discuss the possibility that it is part of the Monoceros tidal stream.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): techniques: spectroscopic - stars: abundances - stars: late-type - globular clusters: general - open clusters and associations: general

VizieR on-line data: <Available at CDS (J/MNRAS/393/272): clusters.dat tables3.dat>

Simbad objects: 587

goto View the reference in ADS


2019.09.23-18:20:47

© Université de Strasbourg/CNRS

    • Contact