High Resolution Spectrum of Symbiotic Star AG Pegasi

Details High Resolution Spectrum of Symbiotic Star AG Pegasi High Resolution Spectrum of Symbiotic Star AG Pegasi

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pkas...21...35y&link_type=abstract

Publications of the Korean Astronomical Society (ISSN 1225-1534), Vol. 21, No. 2, p. 35 - 42 (2006)

Astronomy and Astrophysics

Astronomy

1

High Resolution Spectrum, Slow Nova, Ag Pegasi, Spectral Lines, Geometrical Structure

Scientific paper

We report a high resolution spectrum of AG Pegasi observed at Bohyunsan Optical Astronomy Observatory on October 2, 2004. Some of permitted emission lines, for example H I, He I, He II, Fe II and Ti II were observed in the spectrum of AG Pegasi in 2004. Lines presented in the longer wavelength region than 6500 Å are identified. And radial velocities for each element are measured. Then we carefully discuss the geometrical feature of AG Pegasi in October 2004.

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