About: High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the; Cephei star ; Centauri     Goto   Sponge   NotDistinct   Permalink

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  • We derive the component masses and dynamical parallax of ; Centauri with a precision of 6% and 4%, respectively. Modelling allowed us to refine the mass estimates to 1% precision resulting in M_1=10.7 0.1 M_988857; and M_2=10.3 0.1 M_8857;, and to derive the age of the system as being (14.1 0.6) 106 years. We deduce two oscillation frequencies for the broad-lined primary of 946; Centauri: f_1=7.415 c d-1 and f_2=4.542 c d-1 or one of their aliases. The degrees of these oscillation modes are higher than 2 for both frequencies, irrespective of the alias problem. No evidence of oscillations in the narrow-lined secondary was found.
  • We derive the component masses and dynamical parallax of ; Centauri with a precision of 6% and 4%, respectively. Modelling allowed us to refine the mass estimates to 1% precision resulting in M_1=10.7 0.1 M_988857; and M_2=10.3 0.1 M_8857;, and to derive the age of the system as being (14.1 0.6) 106 years. We deduce two oscillation frequencies for the broad-lined primary of 946; Centauri: f_1=7.415 c d-1 and f_2=4.542 c d-1 or one of their aliases. The degrees of these oscillation modes are higher than 2 for both frequencies, irrespective of the alias problem. No evidence of oscillations in the narrow-lined secondary was found. (en)
  • Hmoty složek a dynamickou paralaxu soustavy jsme určili s přesností 4a6%.Modelování dovolilo zvýšit přesnost určení hmot na 1% na 10,7+- 0,1 a 10,3+-0,1 hmot Slunce a věk soustavy na(14,1+- 0,6) milionů let.Byly zjištěny dvě frekvence oscilací primáru 7,415 a 4,542 cyklů za den. (cs)
Title
  • High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the; Cephei star ; Centauri
  • High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the; Cephei star ; Centauri (en)
  • Vysoce přesné dráhové elementy dvojsložkových spektroskopických dvojhvězd z kombinované interferometrie a spektroskopie.Aplikace na beta Cephei hvězdu beta Centaurí. (cs)
skos:prefLabel
  • High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the; Cephei star ; Centauri
  • High-precision elements of double-lined spectroscopic binaries from combined interferometry and spectroscopy. Application to the; Cephei star ; Centauri (en)
  • Vysoce přesné dráhové elementy dvojsložkových spektroskopických dvojhvězd z kombinované interferometrie a spektroskopie.Aplikace na beta Cephei hvězdu beta Centaurí. (cs)
skos:notation
  • RIV/00216208:11320/06:00002531!RIV07-MSM-11320___
http://linked.open.../vavai/riv/strany
  • 259;269
http://linked.open...avai/riv/aktivita
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  • P(GA205/06/0304), Z(MSM 113200004)
http://linked.open...iv/cisloPeriodika
  • 1
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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  • 477707
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  • RIV/00216208:11320/06:00002531
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • High-precision; elements; double-lined; spectroscopic; binaries; combined; interferometry; spectroscopy; Application; Cephei; Centauri (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [0DB2D5538FE6]
http://linked.open...i/riv/nazevZdroje
  • Astronomy and 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
  • 455
http://linked.open...iv/tvurceVysledku
  • Harmanec, Petr
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://localhost/t...ganizacniJednotka
  • 11320
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