About: HD 161306: a radiatively interacting Be binary?     Goto   Sponge   NotDistinct   Permalink

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  • The spectrum of the Be star HD 161306 is shown to vary periodically with a period close to 100 days. The radial velocity of the He I 6678 A emission peak varying in antiphase to the radial velocity of the Halpha 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 180 km/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.
  • The spectrum of the Be star HD 161306 is shown to vary periodically with a period close to 100 days. The radial velocity of the He I 6678 A emission peak varying in antiphase to the radial velocity of the Halpha 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 180 km/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. (en)
Title
  • HD 161306: a radiatively interacting Be binary?
  • HD 161306: a radiatively interacting Be binary? (en)
skos:prefLabel
  • HD 161306: a radiatively interacting Be binary?
  • HD 161306: a radiatively interacting Be binary? (en)
skos:notation
  • RIV/67985815:_____/14:00433681!RIV15-GA0-67985815
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(GA14-21373S), P(GAP209/10/0715), P(LG14026)
http://linked.open...iv/cisloPeriodika
  • July
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 18822
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/14:00433681
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • binaries: spectroscopic; stars: emission-line; Be: stars (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [BEA1E0C28450]
http://linked.open...i/riv/nazevZdroje
  • Astronomy & Astrophysics
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 567
http://linked.open...iv/tvurceVysledku
  • Votruba, Viktor
  • Škoda, Petr
  • Šlechta, Miroslav
  • Kotková, Lenka
  • Koubský, Pavel
  • Kraus, Michaela
  • Harmanec, P.
  • Wolf, M.
  • Kubát, Jiří
  • Yang, S.
  • Kubátová, Brankica
  • Niemczura, E.
http://linked.open...ain/vavai/riv/wos
  • 000341185300144
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201424022
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