Ionization states and cooling efficiencies

DOI

We present new computations of the equilibrium and nonequilibrium cooling efficiencies and ionization states for low-density radiatively cooling gas containing the elements H, He, C, N, O, Ne, Mg, Si, S, and Fe. We present results for gas temperatures between 10^4^ and 10^8^K, assuming dust-free and optically thin conditions, and no external radiation.

Identifier
DOI http://doi.org/10.26093/cds/vizier.21680213
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJS/168/213
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/168/213
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/168/213
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJS/168/213
Provenance
Creator Gnat O.; Sternberg A.
Publisher CDS
Publication Year 2009
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; Galactic and extragalactic Astronomy; High Energy Astrophysics; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy