Catalog Service: O abundances from HARPS in F-G stars
Description
We present a detailed and uniform study of oxygen abundance from two different oxygen lines at 6158{AA} and 6300{AA} in a large sample of solar-type stars. The results are used to check the behaviour of these spectral lines as oxygen abundance indicators and to study the evolution of oxygen in thick and thin disk populations of the Galaxy. Equivalent width measurements were carried out for the [OI]6158 and [OI]6300 lines. LTE abundances were obtained from these two lines in 610 and 535 stars, respectively. Careful error analysis has been performed.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2015 Apr 09 08:59:20ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/A+A/576/A89/o6158 (Stellar parameters, EW and [O/H] and statistical results for O{lambda}6158{AA})
VERB=1
VERB=3
Cone search capability for table J/A+A/576/A89/o6300 (Stellar parameters, EW and [O/H] and statistical results for O{lambda}6300{AA})
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
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