Spectroscopic Study of 31 Cygni

Details Spectroscopic Study of 31 Cygni Spectroscopic Study of 31 Cygni

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jass....8...25s&link_type=abstract

Journal of Astronomy and Space Sciences, vol.8, no1, p.25-51.

Astronomy and Astrophysics

Astronomy

Scientific paper

The spectra of 31 Cygni were taken at the Asiago Observatory in Italy. Reduction was made using the 2nd and 4th order non-linear least square method. Spectral lines which were relatively sharp or strang were identified within the wavelength regions from 3800 to 5100 Å. Radial velocities and equivalent widths were calculated from the Gaussian Fitting Method for this star. The measured mean radial velocity of 31 Cygni is +0.5 km/sec.

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