Main-sequence star chromospheres Virtual Observatory Resource

Authors
  1. Houdebine E.R.
  2. Published by
    CDS
Abstract

We report on high-resolution observations of two dM1 stars: Gl 867A, an active dM1e star, and Gl 205, a less active dM1 star. The wavelength coverage is from 3890 to 6820{AA} with a resolving power of about 45000. The difference spectrum of these two stars allows us to make a survey of spectral lines sensitive to magnetic activity.

Keywords
  1. late-type-stars
  2. magnetic-fields
  3. spectroscopy
Bibliographic source Bibcode
2010MNRAS.403.2157H
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/403/2157
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/403/2157

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/403/2157
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/403/2157
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/403/2157
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2010-11-26T14:44:01Z
Resource record created
2010-11-26T14:44:01Z
Created
2015-06-10T12:36:29Z
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