Emission lines in a giant flare of CN Leo Virtual Observatory Resource

Authors

1. Fuhrmeister B.
2. Liefke C.
3. Schmitt J.H.M.M.
4. Reiners A.

Published by

CDS

Abstract

Flares on dM stars contain plasmas at very different temperatures and thus affect a wide wavelength range in the electromagnetic spectrum. While the coronal properties of flares are studied best in X-rays, the chromosphere of the star is observed best in the optical and ultraviolet ranges. Therefore, multiwavelength observations are essential to study flare properties throughout the atmosphere of a star.

Keywords

1. late-type-stars
2. m-stars

Bibliographic source Bibcode

2008A&A...487..293F

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/487/293

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/487/293

Document Object Identifer DOI

doi:10.26093/cds/vizier.34870293

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/487/293
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/487/293
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/487/293

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).