SPECTRAL BEHAVIORS OF Hβ LINE OF CH CYGNI IN A QUIESCENT PHASE

SPECTRAL BEHAVIORS OF Hβ LINE OF CH CYGNI IN A QUIESCENT PHASE

We analyzed the high resolution H,6 line spectra of CH Cygni obtained at the Bohyunsan Astronomical Observatory (BOAO) on April 2004. The temporal changes in the Hβ line profiles are reported. We obtained the equivalent widths of the Gaussian components. Using this we estimated the length of the gas...

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Veröffentlicht in:Publications of The Korean Astronomical Society 2004-12, Vol.19 (1), p.21-25
Hauptverfasser: YOO, KYE HWA, KIM, KANG MIN, LEE, BYUNG CHUL, YOON, TAE SEOG, LEE, JUNG AE
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container_title Publications of The Korean Astronomical Society
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creator YOO, KYE HWA
KIM, KANG MIN
LEE, BYUNG CHUL
YOON, TAE SEOG
LEE, JUNG AE
description We analyzed the high resolution H,6 line spectra of CH Cygni obtained at the Bohyunsan Astronomical Observatory (BOAO) on April 2004. The temporal changes in the Hβ line profiles are reported. We obtained the equivalent widths of the Gaussian components. Using this we estimated the length of the gaseous nebula which emits the Hβ line and the mass loss rate from the star.
doi_str_mv 10.5303/PKAS.2004.19.1.021
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title SPECTRAL BEHAVIORS OF Hβ LINE OF CH CYGNI IN A QUIESCENT PHASE
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