Variations of the fine-structure constant Virtual Observatory Resource

Authors
  1. Murphy M.T.
  2. Webb J.K.
  3. Flambaum V.
  4. Published by
    CDS
Abstract

The Keck telescope's High Resolution Spectrograph (HIRES) has previously provided evidence for a smaller fine-structure constant, {alpha}, compared to the current laboratory value, in a sample of 143 quasar absorption systems: {Delta}{alpha}/{alpha}=(-0.57+/-0.11)10^-5^. The analysis was based on a variety of metal-ion transitions which, if alpha varies, experience different relative velocity shifts. This result is yet to be robustly contradicted, or confirmed, by measurements on other telescopes and spectrographs; it remains crucial to do so.

Keywords
  1. atomic-physics
  2. quasars
Bibliographic source Bibcode
2009MmSAI..80..833M
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/MmSAI/80.833
IVOA Identifier IVOID
ivo://CDS.VizieR/J/other/MmSAI/80.833

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/MmSAI/80.833
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/MmSAI/80.833
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/MmSAI/80.833
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/other/MmSAI/80.833/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/other/MmSAI/80.833/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/other/MmSAI/80.833/table1?

History

2010-03-09T07:42:31Z
Resource record created
2010-03-09T07:42:31Z
Created
2018-11-05T10:52:51Z
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