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  • We studied both components of a slightly overlooked visual binary HR 1847 spectroscopically to determine its basic physical and orbital parameters. Basic stellar parameters were determined by comparing synthetic spectra to the observed echelle spectra, which cover both the optical and near-IR regions. New observations of this system used the Ondrejov and Rozhen 2-m telescopes and their coude spectrographs. Radial velocities from individual spectra were measured and then analysed with the code FOTEL to determine orbital parameters. The spectroscopic orbit of HR 1847A is presented for the first time. It is a single-lined spectroscopic binary with a B-type primary, a period of 719.79 days, and a highly eccentric orbit with e = 0.7. We confirmed that HR 1847B is a Be star. Its Ha emission significantly decreased from 2003 to 2008. Both components have a spectral type B7-8 and luminosity class IV-V.
  • We studied both components of a slightly overlooked visual binary HR 1847 spectroscopically to determine its basic physical and orbital parameters. Basic stellar parameters were determined by comparing synthetic spectra to the observed echelle spectra, which cover both the optical and near-IR regions. New observations of this system used the Ondrejov and Rozhen 2-m telescopes and their coude spectrographs. Radial velocities from individual spectra were measured and then analysed with the code FOTEL to determine orbital parameters. The spectroscopic orbit of HR 1847A is presented for the first time. It is a single-lined spectroscopic binary with a B-type primary, a period of 719.79 days, and a highly eccentric orbit with e = 0.7. We confirmed that HR 1847B is a Be star. Its Ha emission significantly decreased from 2003 to 2008. Both components have a spectral type B7-8 and luminosity class IV-V. (en)
Title
  • Spectroscopic analysis of the B/Be visual binary HR 1847
  • Spectroscopic analysis of the B/Be visual binary HR 1847 (en)
skos:prefLabel
  • Spectroscopic analysis of the B/Be visual binary HR 1847
  • Spectroscopic analysis of the B/Be visual binary HR 1847 (en)
skos:notation
  • RIV/67985815:_____/10:00354857!RIV11-GA0-67985815
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/08/0003), Z(AV0Z10030501)
http://linked.open...iv/cisloPeriodika
  • Sep-Oct
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
  • 289152
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/10:00354857
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Be stars; emission-line (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [00403C7B9614]
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
  • 520
http://linked.open...iv/tvurceVysledku
  • Dovčiak, Michal
  • Hadrava, Petr
  • Kawka, Adela
  • Korčáková, Daniela
  • Votruba, Viktor
  • Škoda, Petr
  • Šlechta, Miroslav
  • Kubát, Jiří
  • Iliev, L.
  • Saad, S. M.
  • Nouh, M. I.
  • Uytterhoeven, K.
http://linked.open...ain/vavai/riv/wos
  • 000283064200086
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
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