Space photometry of the Be stars nu Pup

DOI

Photometry of the bright Be star {nu} Puppis. The observations were obtained with the Solar Mass Ejection Imager (SMEI) and BRITE-Constellation satellites. Several closely but probably not perfectly evenly spaced frequencies are found that are attributed to nonradial pulsations.

Identifier
DOI http://doi.org/10.26093/cds/vizier.36200145
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/620/A145
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/620/A145
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/620/A145
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/620/A145
Provenance
Creator Baade D.; Pigulski A.; Rivinius T.; Wang L.; Martayan C.; Handler G.,Panoglou D.; Carciofi A.C.; R.Kuschnig; Mehner A.; Moat A.F.J.; Pablo H.,Rucinski S.M.; Wade G.A.; Weiss W.W.; Zwintz K.
Publisher CDS
Publication Year 2018
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; Observational Astronomy; Physics; Stellar Astronomy