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  • TW Draconis is one of the most well known interacting Algol-type eclipsing binaries. We study time series data for the star accumulated over the past 150 years to detect changes in minima timings. Using 561 available minima timings, we compile an extended O-C diagram analysis. The first part ending around 1942 is characterised by smooth linear/parabolic course of timing residuals. In 1858-1905, the period was almost constant P=2.806513(9)d, but, in 1905-1942, the period increased. We interpret it as a result of continuous mass exchange at the mean rate of 6.9x10^-7 Ms year-1. Since 1942, the system has been showing alternating and shortening period changes with the length of a cycle of about two decades, modulated by short-term periodic variations. The latter small variations with the period 6.5 years are caused by the the presence of a third low-mass body in the system. Major oscillations can be explained as consequences of quadrupole moment variation in the system.
  • TW Draconis is one of the most well known interacting Algol-type eclipsing binaries. We study time series data for the star accumulated over the past 150 years to detect changes in minima timings. Using 561 available minima timings, we compile an extended O-C diagram analysis. The first part ending around 1942 is characterised by smooth linear/parabolic course of timing residuals. In 1858-1905, the period was almost constant P=2.806513(9)d, but, in 1905-1942, the period increased. We interpret it as a result of continuous mass exchange at the mean rate of 6.9x10^-7 Ms year-1. Since 1942, the system has been showing alternating and shortening period changes with the length of a cycle of about two decades, modulated by short-term periodic variations. The latter small variations with the period 6.5 years are caused by the the presence of a third low-mass body in the system. Major oscillations can be explained as consequences of quadrupole moment variation in the system. (en)
Title
  • Period study of TW Draconis
  • Period study of TW Draconis (en)
skos:prefLabel
  • Period study of TW Draconis
  • Period study of TW Draconis (en)
skos:notation
  • RIV/00216224:14310/08:00025155!RIV10-GA0-14310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/04/2063), P(GA205/06/0217), Z(MSM0021620860)
http://linked.open...iv/cisloPeriodika
  • 1
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
  • 386276
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/08:00025155
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • stars: binaries: eclipsing; stars: individual: TW Dra; stars: fundamental parameters (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [D9D7BC2E379C]
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
  • 489
http://linked.open...iv/tvurceVysledku
  • Mikulášek, Zdeněk
  • Zejda, Miloslav
  • Wolf, Marek
http://linked.open...ain/vavai/riv/wos
  • 000259347400027
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://localhost/t...ganizacniJednotka
  • 14310
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