Manganese abundances in the Galactic disk

DOI

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.

Cone search capability for table J/A+A/467/665/table1 (Stellar parameters for the stars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34670665
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/467/665
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/467/665
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/467/665
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/467/665
Provenance
Creator Feltzing S.; Fohlman M.; Bensby T.
Publisher CDS
Publication Year 2007
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics; Stellar Astronomy