Spectral line identification in 3 Pup

Optical spectra taken in 1997-2008 are used to analyze the spectral peculiarities and velocity field in the atmosphere of the peculiar supergiant 3 Pup.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/other/AstBu/65.150
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/AstBu/65.150
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/AstBu/65.150
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/other/AstBu/65.150
Provenance
Creator Chentsov E.L.; Klochkova V.G.; Miroshnichenko A.S.
Publisher CDS
Publication Year 2010
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; Exoplanet Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy