BD+33 2642 and HD 112313 radial velocities

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35639010
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/563/L10
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/563/L10
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/563/L10
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/563/L10
Provenance
Creator Van Winckel H.; Jorissen A.; Exter K.; Raskin G.; Prins S.,Perez Padilla J.; Merges F.; Pessemier W.
Publisher CDS
Publication Year 2014
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 Astrophysical Processes; Astrophysics and Astronomy; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy