LTE spectrum synthesis in magnetic atmospheres

DOI

Files table4.dat contain calculated Stokes IQUV local line profiles of Fe II 4923.9 shown in Fig. 4 of this paper. Profile sets are provided for 0.1, 5 and 20kG magnetic fields, with vector orientation {psi}=40{deg}, {phi}=0{deg}, disc centre and eps_fe_=4.6.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33740265
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/374/265
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/374/265
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/374/265
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/374/265
Provenance
Creator Wade G.A.; Bagnulo S.; Kochukhov O.; Landstreet J.D.; Piskunov N.,Stift M.J.
Publisher CDS
Publication Year 2001
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 Astrophysical Processes; Astrophysics and Astronomy; Exoplanet Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy