IUE Archival Spectra of 31 Cygni

Details IUE Archival Spectra of 31 Cygni IUE Archival Spectra of 31 Cygni

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jass....8...53k&link_type=abstract

Journal of Astronomy and Space Sciences, vol.8, no1, p.53-61.

Astronomy and Astrophysics

Astronomy

Scientific paper

UV light curve of 31 Cygni has been made from the IUE high dispersion spectra. The depth of primary minimum of the light curve is 5.2 magnitudes because the B4 star's steep spectral gradient. The light curve has been analyzed by the method of Wilson and Devinney Differential Correction(WD). The radial velocities have been measured using the Mg ¥± h lines. The spectroscopic elements have been determined by the method of WD. The change of the Mg ¥± resonance doublet has been investigated based on the eight representative spectra taken at well distributed orbital phases.

Affiliated with

Also associated with

No associations

Rating

IUE Archival Spectra of 31 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 IUE Archival Spectra of 31 Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IUE Archival Spectra of 31 Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1284368