Manganese abundances in the Galactic disk Virtual Observatory Resource

Authors

1. Feltzing S.
2. Fohlman M.
3. Bensby T.

Published by

CDS

Abstract

Manganese is an iron-peak element and although the nucleosynthesis path that leads to its formation is fairly well understood, it remains unclear which objects, SN II and/or SN Ia, that contribute the majority of Mn to the interstellar medium. It also remains unclear to which extent the supernovae Mn yields depend on the metallicity of the progenitor star or not.

Keywords

1. late-type-stars
2. chemical-abundances

Bibliographic source Bibcode

2007A&A...467..665F

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/467/665

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/467/665

Document Object Identifer DOI

doi:10.26093/cds/vizier.34670665

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/467/665
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/467/665
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/467/665

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Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/467/665/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/467/665/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/467/665/table1?