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

Authors
  1. Hinkle K.H.
  2. Wallace L.
  3. Ram R.S.
  4. Bernath P.F.
  5. Sneden C.
  6. Lucatello S.
  7. Published by
    CDS
Abstract

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.

Keywords
  1. atomic-physics
  2. spectroscopy
Bibliographic source Bibcode
2013ApJS..207...26H
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/207/26
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJS/207/26
Document Object Identifer DOI
doi:10.26093/cds/vizier.22070026

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/207/26
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/207/26
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/207/26
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2013-10-07T10:35:04Z
Resource record created
2013-10-07T10:35:04Z
Created
2017-06-21T08:22:24Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr