Dust formation in WC stars

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33570572
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/357/572
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/357/572
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/357/572
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/357/572
Provenance
Creator Cherchneff I.; Le Teuff Y.H.; Williams P.M.; Tielens A.G.G.M.
Publisher CDS
Publication Year 2000
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy