Space photometry of the Be stars nu Pup Virtual Observatory Resource

Authors

1. Baade D.
2. Pigulski A.
3. Rivinius T.
4. Wang L.
5. Martayan C.
6. Handler G.,Panoglou D.
7. Carciofi A.C.
8. R.Kuschnig
9. Mehner A.
10. Moat A.F.J.
11. Pablo H.,Rucinski S.M.
12. Wade G.A.
13. Weiss W.W.
14. Zwintz K.

Published by

CDS

Abstract

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.

Keywords

1. Emission line stars
2. Be stars
3. Early-type stars
4. Apparent magnitude
5. Optical astronomy

Bibliographic source Bibcode

2018A&A...620A.145B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/620/A145

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/620/A145

Document Object Identifer DOI

doi:10.26093/cds/vizier.36200145

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/620/A145
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/620/A145
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/620/A145

IVOA Table Access TAP

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