M ¥± Line Variation of 32 Cygni

Details M ¥± Line Variation of 32 Cygni M ¥± Line Variation of 32 Cygni

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jass....9..154k&link_type=abstract

Journal of Astronomy and Space Sciences, vol.9, no.2, 154-164.

Astronomy and Astrophysics

Astronomy

Scientific paper

The Mg ¥± lines have been extracted from the IUE archival spectra of 32 Cygni to investigate the effect of the atmospheric eclipse. The UV light curve has been reduced from the continuum flux at the center wavelength of 2807.5 Å in the IUE spectra. The equivalent width of the Mg ¥± k absoption line has been measured for each spectra. The results of the light variation and flux tracing of the absorption line at the vicinity of the primary eclipse confirmed the atmospheric eclipse. The atmospheric effect lasted until the phase 0.06 in the absorptin line tracing, while it lasted until the phase 0.02 in the UV light curve, respectively.

Affiliated with

Also associated with

No associations

Rating

M ¥± Line Variation of 32 Cygni does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with M ¥± Line Variation of 32 Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and M ¥± Line Variation of 32 Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1115412