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Table · dataset · 2009

Equivalent widths of IC 2602 & IC 2391 stars

Listed in IVOA Registry (Virtual Observatory)

Galactic open clusters have been long recognized as one of the best tools to investigate the chemical content of Galactic disk and its time evolution.

Description

In the last decade, many efforts have been directed to chemically characterize the old and intermediate age population; surprisingly, the chemical content of the younger and close counterpart remains largely undetermined. In this paper we present the abundance analysis of a sample of 15 G/K members of the young pre-main sequence clusters IC 2602 and IC 2391.

Along with IC 4665, these are the first pre-main sequence clusters for which a detailed abundance determination has been carried out so far.

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Documentation and papers

Catalogue records · 2

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Optical
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Astronomical sciences 73%
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/501/55311 d agoJSON v1
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concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
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license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
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updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0