BD+33 2642 and HD 112313 radial velocities Virtual Observatory Resource

Authors

1. Van Winckel H.
2. Jorissen A.
3. Exter K.
4. Raskin G.
5. Prins S.,Perez Padilla J.
6. Merges F.
7. Pessemier W.

Published by

CDS

Abstract

We study the impact of binary interaction processes on the evolution of low- and intermediate-mass stars using long-term monitoring of their radial velocity. Here we report on our results on the central stars of two planetary nebulae (PNe): the well-studied spectrophotometric standard BD+33 2642 (central star of PNG 052.7+50.7) and HD 112313 (central star of PN LoTr5), the optical light of which is dominated by a rapidly rotating G star.

Keywords

1. orbits
2. spectroscopic-binary-stars
3. planetary-nebulae
4. spectroscopy

Bibliographic source Bibcode

2014A&A...563L..10V

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/563/L10

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/563/L10

Document Object Identifer DOI

doi:10.26093/cds/vizier.35639010

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/563/L10
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/563/L10
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/563/L10

IVOA Table Access TAP

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