Emission Lines in 32 Cygni

Details Emission Lines in 32 Cygni Emission Lines in 32 Cygni

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jad....14....3e&link_type=abstract

The Journal of Astronomical Data

Other

32 Cyg, Spectroscopy

Scientific paper

I identify the profusion of emission lines seen in IUE spectra of 32 Cyg (K4-5 Ib+B6-7 IV-V) during total eclipse. With the exception of a very few weak lines, all of these are also seen in zeta Aur during its eclipse, and the stronger features appear in 31 Cyg. Seventy-four percent of these emission lines can be attributed to Fe II. Few are intrisically weaker than gf~0.01. Other spectra definitely present are C II, N I, O I, Si II, Mg II, S II, Cr II, Ni II, Al II, Al III, F III, Si IV, and C IV. No emission lines of the neutral metals, except for fluorescent Fe I UV44, are unambiguously detected; specifically, lines of C I, Si I, or S I were not detected in the spectrum.

Affiliated with

Also associated with

No associations

Rating

Emission Lines in 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 Emission Lines in 32 Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emission Lines in 32 Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-747975