Dust formation in WC stars Virtual Observatory Resource

Authors

1. Cherchneff I.
2. Le Teuff Y.H.
3. Williams P.M.
4. Tielens A.G.G.M.

Published by

CDS

Abstract

The following table gives the ratefile of the chemical model. Columns {alpha}, {beta} and {gamma} give the rate k at temperature T in the Arrhenius form: k = {alpha} * (T/300)^{beta}^ * exp(-{gamma}/T) The arrows indicate reversible reactions.

Keywords

1. wolf-rayet-stars
2. carbon-stars
3. stellar-evolutionary-models

Bibliographic source Bibcode

2000A&A...357..572C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/357/572

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/357/572

Document Object Identifer DOI

doi:10.26093/cds/vizier.33570572

Access

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IVOA Table Access TAP

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