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Table · dataset · 2008

Scaled solar tracks and isochrones

Listed in IVOA Registry (Virtual Observatory)

In many astrophysical contexts, the helium content of stars may differ significantly from those usually assumed in evolutionary calculations.

Description

In order to improve upon this situation, we have computed tracks and isochrones in the range of initial masses 0.15-20M_{sun}_ for a grid of 39 chemical compositions with the metal content Z between 0.0001 and 0.070 and helium content Y between 0.23 and 0.46. **************************************************************************

  • *
  • Sorry, but the author(s) never supplied the tabular material
  • * announced in the paper
  • *
  • **************************************************************************

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Catalogue records · 2

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Inferred from text
Tabular 75%
Provenance · 1 source records, 8 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/484/81511 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].local:modality:tabularenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (75%)
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