LTE spectrum synthesis in magnetic atmospheres Virtual Observatory Resource

Authors

1. Wade G.A.
2. Bagnulo S.
3. Kochukhov O.
4. Landstreet J.D.
5. Piskunov N.,Stift M.J.

Published by

CDS

Abstract

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.

Keywords

1. astronomical-models
2. stellar-atmospheres
3. magnetic-fields
4. spectroscopy
5. polarimetry

Bibliographic source Bibcode

2001A&A...374..265W

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/374/265

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/374/265

Document Object Identifer DOI

doi:10.26093/cds/vizier.33740265

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/374/265
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/374/265
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/374/265

IVOA Table Access TAP

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