Emission lines in a flare of AB Dor A Virtual Observatory Resource

Authors
  1. Lalitha S.
  2. Fuhrmeister B.
  3. Wolter U.
  4. Schmitt J.H.M.M.
  5. Engels D.,Wieringa M.H.
  6. Published by
    CDS
Abstract

We present a identification catalog of chromospheric emission lines in the optical range for two flares on AB Dor A, with event 1 being larger than event 3. An additional flare event 2 is not described here because of its overlap with event 1. All lines are identified in an flare- only spectrum, i.e. with a quiescent spectrum subtracted. The data were obtained with ESO's Kueyen telescope equipped with the UVES spectrograph on November 25/26 in 2009. The instrument was operated in dichroic mode (spectral coverage from 3720 to 4945 and from 5695 to 9465 AA). We tabulate measured wavelength, line flux and FWHM for every line and also provide the rest wavelength from the Moore catalog which was used for identification (Moore, 1972, Nat. Stand. Ref. Data. Ser., 40). Few lines were identified with the NIST database.

Keywords
  1. variable-stars
  2. m-stars
  3. spectroscopy
Bibliographic source Bibcode
2013A&A...560A..69L
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/560/A69
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/560/A69
Document Object Identifer DOI
doi:10.26093/cds/vizier.35600069

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/560/A69
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/560/A69
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/560/A69
IVOA Table Access TAP
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Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2013-12-06T09:15:30Z
Resource record created
2013-12-06T09:15:30Z
Created
2017-07-12T06:59:39Z
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