SIMBAD references

2012A&A...544A.109C - Astronomy and Astrophysics, volume 544A, 109-109 (2012/8-1)

Radial velocities and metallicities from infrared Ca II triplet spectroscopy of open clusters. Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266.

CARRERA R.

Abstract (from CDS):

Open clusters are ideal test particles for studying the formation and evolution of the Galactic disk. However, the number of clusters with information about their radial velocities and chemical compositions remains largely insufficient. We attempt to increase the number of open clusters with determinations of radial velocities and metallicities from spectroscopy. We acquired medium-resolution spectra (R∼8000) in the region of the infrared CaII triplet lines (∼8500Å) for several stars in four open clusters with the long-slit spectrograph IDS at the 2.5m Isaac Newton Telescope, Roque de los Muchachos Observatory, Spain. Radial velocities were obtained by cross-correlating the observed spectra with those of two template stars. We used the relationships available in the literature between the strength of infrared CaII lines and metallicities to derive the metal content of each cluster. We provide the first spectroscopic determinations of radial velocities and metallicities for the open clusters Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266. We obtain <Vr≥68±12, -15±7, 2±10, and -16±15km/s for Berkeley 26, Berkeley 70, NGC 1798, and NGC 2266, respectively. For Berkeley 26 we derive a metallicity of [Fe/H]=-0.35±0.17dex. Berkeley 70 has a solar metallicity of [Fe/H]=-0.01±0.14dex, while NGC 1798 has a slightly lower metal content of [Fe/H]=-0.12±0.07dex. Finally, we derive a metallicity of [Fe/H]=-0.38±0.06dex for NGC 2266.

Abstract Copyright:

Journal keyword(s): open clusters and associations: individual: Berkeley 26 - open clusters and associations: individual: Berkeley 70 - open clusters and associations: individual: NGC 1798 - open clusters and associations: individual: NGC 2266 - stars: abundances - Galaxy: disk

Status in Simbad:  being processed

CDS comments: In Table 1 stars in Be 70 are Cl* Berkeley 70 HMK NNN in SIMBAD, not with numbers in column 2. Stars in NGC 1798 are Cl* NGC 1798 PL NN with the same numerotation except Star 608 (2MASS J05114094+4740431 in SIMBAD). Stars in NGC 2266 are Cl* NGC 2266 C NN in SIMBAD, except 1011 (Cl* NGC 2266 KM 11 in SIMBAD).

Simbad objects: 10

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2019.12.07-12:58:44

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