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Table · dataset · 2006

Grid of close binaries experiencing mass exchange

Listed in IVOA Registry (Virtual Observatory)

To simulate the population of the primordial blue stragglers in old open clusters, a grid of close binaries experiencing mass exchange is needed.

Description

To this aim, various combinations that can trigger mass exchange for the donor masses of 0.1M_{sun}_ to 2.0M_{sun}_ are calculated with a fine grid in parameters. The mass range of the accretor is from 0.1M_{sun}_ to the mass of the corresponding donor.

The mass intervals of the donors and the accretors are all 0.1M_{sun}_. To cover all possible cases of close binaries, the orbit separation ranges from 1.0 to 50.0R_{sun}_ with a grid interval of 1.0R_{sun}_. Following the numerical scheme described above, a grid for six ages from 1.0Gyr to 6.0Gyr is obtained.

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In this table, mass, effective temperature, luminosity, gravity, Hydrogen abundance in the core, Helium abundance in the core, B magnitude, V magnitude, B-V color, mass ratio, orbital separation and period of the close binaries experiencing mass exchange are given.

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Catalogue records · 2

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Provenance · 1 source records, 8 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/455/24712 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 (65%)
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