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Table · dataset · 2014

Evolution of rotating very massive LC stars

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With growing evidence for the existence of very massive stars at subsolar metallicity, there is an increased need for corresponding stellar evolution models.

Description

We present a dense model grid with a tailored input chemical composition appropriate for the Large Magellanic Cloud (LMC).

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Catalogue records · 2

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Astronomical sciences 74%
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/573/a7114 d agoJSON v1
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concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (74%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0