MgH in the A^2^{Pi}-X^2^{Sigma}^+^ system

DOI

Using laboratory hollow cathode spectra we have identified lines of the less common magnesium isotopologues of MgH, ^25^MgH and ^26^MgH, in the A^2^{Pi}-X^2^{Sigma}^+^ system. Based on the previous analysis of ^24^MgH, molecular lines have been measured and molecular constants derived for ^25^MgH and ^26^MgH. Term values and linelists, in both wavenumber and wavelength units, are presented. The A^2^{Pi}-X^2^{Sigma}^+^ system of MgH is important for measuring the magnesium isotope ratios in stars.

Identifier
DOI http://doi.org/10.26093/cds/vizier.22070026
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJS/207/26
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/207/26
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/207/26
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJS/207/26
Provenance
Creator Hinkle K.H.; Wallace L.; Ram R.S.; Bernath P.F.; Sneden C.; Lucatello S.
Publisher CDS
Publication Year 2013
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; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics