Emission lines in a giant flare of CN Leo

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34870293
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/487/293
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/487/293
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/487/293
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/487/293
Provenance
Creator Fuhrmeister B.; Liefke C.; Schmitt J.H.M.M.; Reiners A.
Publisher CDS
Publication Year 2008
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Physics; Stellar Astronomy