About: Molecular emission from GG Carinae's circumbinary disk     Goto   Sponge   NotDistinct   Permalink

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  • We aim at studying the kinematics and origin of the disk in the eccentric binary system GG Car, whose primary component is proposed to be a B[e] supergiant. We find that the CO gas is located in a ring surrounding the eccentric binary system, and its kinematics agrees with Keplerian rotation with a velocity, projected to the line of sight, of 80 +/- 1 km s(-1). The CO ring has a column density of (5 +/- 3) x 10(21) cm(-2) and a temperature of 3200 +/- 500 K. In addition, the material is chemically enriched in C-13, which agrees with the primary component being slightly evolved off the main sequence. We discuss two possible scenarios for the origin of the circumbinary disk: (i) non-conservative Roche lobe overflow; and (ii) the possibility that the progenitor of the primary component could have been a classical Be star. Neither can be firmly excluded, but for Roche lobe overflow to occur, a combination of stellar and orbital parameter extrema would be required.
  • We aim at studying the kinematics and origin of the disk in the eccentric binary system GG Car, whose primary component is proposed to be a B[e] supergiant. We find that the CO gas is located in a ring surrounding the eccentric binary system, and its kinematics agrees with Keplerian rotation with a velocity, projected to the line of sight, of 80 +/- 1 km s(-1). The CO ring has a column density of (5 +/- 3) x 10(21) cm(-2) and a temperature of 3200 +/- 500 K. In addition, the material is chemically enriched in C-13, which agrees with the primary component being slightly evolved off the main sequence. We discuss two possible scenarios for the origin of the circumbinary disk: (i) non-conservative Roche lobe overflow; and (ii) the possibility that the progenitor of the primary component could have been a classical Be star. Neither can be firmly excluded, but for Roche lobe overflow to occur, a combination of stellar and orbital parameter extrema would be required. (en)
Title
  • Molecular emission from GG Carinae's circumbinary disk
  • Molecular emission from GG Carinae's circumbinary disk (en)
skos:prefLabel
  • Molecular emission from GG Carinae's circumbinary disk
  • Molecular emission from GG Carinae's circumbinary disk (en)
skos:notation
  • RIV/67985815:_____/13:00399497!RIV14-GA0-67985815
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • I, P(GAP209/11/1198)
http://linked.open...iv/cisloPeriodika
  • January
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
  • Kraus, Michaela
  • Aret, Anna
  • Oksala, Mary E.
  • Nickeler, Dieter Horst
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 89308
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/13:00399497
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars; emission-line; Be stars (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [48A640FAEFA6]
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
  • 549
http://linked.open...iv/tvurceVysledku
  • Borges Fernandes, M.
  • Kraus, Michaela
  • Aret, Anna
  • Muratore, M. F.
  • Cidale, L. S.
  • Oksala, Mary E.
  • Nickeler, Dieter Horst
  • de Wit, A. J.
http://linked.open...ain/vavai/riv/wos
  • 000313745000028
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201220442
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