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Description
  • The ephemeris of variations of the cool magnetic CP star HD188041 was newly determined using all photometric, magnetic and spectroscopic observations available. The improved period P=(223.826+-0.040)d is common for all type of variations observed, the other ever mentioned periods were definitely eliminated. The origin of phase counting M0 = 2,444,981.8+-0.6 was put in the center of v light minimum. The effective magnetic field maximum lies at the phase 0.002+-0.019. The slightly asymmetric curve of Gd II line intensity has its maximum at -0.031+-0.012.
  • The ephemeris of variations of the cool magnetic CP star HD188041 was newly determined using all photometric, magnetic and spectroscopic observations available. The improved period P=(223.826+-0.040)d is common for all type of variations observed, the other ever mentioned periods were definitely eliminated. The origin of phase counting M0 = 2,444,981.8+-0.6 was put in the center of v light minimum. The effective magnetic field maximum lies at the phase 0.002+-0.019. The slightly asymmetric curve of Gd II line intensity has its maximum at -0.031+-0.012. (en)
  • The ephemeris of variations of the cool magnetic CP star HD188041 was newly determined using all photometric, magnetic and spectroscopic observations available. The improved period P=(223.826+-0.040)d is common for all type of variations observed, the other ever mentioned periods were definitely eliminated. The origin of phase counting M0 = 2,444,981.8+-0.6 was put in the center of v light minimum. The effective magnetic field maximum lies at the phase 0.002+-0.019. The slightly asymmetric curve of Gd II line intensity has its maximum at -0.031+-0.012. (cs)
Title
  • Improved period of a slowly rotating cool magnetic CP star HD 188 041
  • Improved period of a slowly rotating cool magnetic CP star HD 188 041 (en)
  • Improved period of a slowly rotating cool magnetic CP star HD 188 041 (cs)
skos:prefLabel
  • Improved period of a slowly rotating cool magnetic CP star HD 188 041
  • Improved period of a slowly rotating cool magnetic CP star HD 188 041 (en)
  • Improved period of a slowly rotating cool magnetic CP star HD 188 041 (cs)
skos:notation
  • RIV/00216224:14310/03:00007927!RIV08-MSM-14310___
http://linked.open.../vavai/riv/strany
  • 29-37
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/02/0445), P(ME 131)
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
  • 609971
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/03:00007927
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • CP star; HD 188 041; magnetic star; uvby photometry; period (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • SK - Slovenská republika
http://linked.open...ontrolniKodProRIV
  • [1D9773699003]
http://linked.open...i/riv/nazevZdroje
  • Contributions of the Astronomical Observatory Skalnaté Pleso
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
  • 33
http://linked.open...iv/tvurceVysledku
  • Mikulášek, Zdeněk
  • Zverko, Juraj
  • Žižňovský, Jozef
  • Polosukhina, Nina S.
issn
  • 1335-1842
number of pages
http://localhost/t...ganizacniJednotka
  • 14310
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