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Resource Record Summary

Catalog Service:
HD 161306 H{alpha} and HeI spectra

Short name: J/A+A/567/A57
IVOA Identifier: ivo://CDS.VizieR/J/A+A/567/A57
DOI (Digital Object Identifier): 10.26093/cds/vizier.35670057
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/567/A57
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2014 Jul 10 11:15:11Z
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Description


The spectrum of the Be star HD 161306 is shown to vary periodically with a period of ~100-days. The radial velocity of the HeI 6678{AA} emission peak varying in antiphase to the radial velocity of the H{alpha} emission wings component suggests that the star is a binary similar to {phi} Per, 59 Cyg, or FY CMa, i.e. a radiatively interacting Be binary - a rare case among Be stars. This type of object is also called a {phi} Per-type binary or Be + sdO binaries. The range of radial-velocity variations of the strong emission peak in the helium line observed in HD 161306 is about 180km/s, similar to what is observed for these systems. We therefore conclude that HD 161306 may represent another case of a Be star with a hot subdwarf companion.

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