Spectral observations of CH Cyg. II - Emission lines from 1978 to 1982

Details Spectral observations of CH Cyg. II - Emission lines from 1978 to 1982 Spectral observations of CH Cyg. II - Emission lines from 1978 to 1982

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...77r&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Nov.-Dec. 1986, p. 77-82. In Russian.

Physics

Cygnus Constellation, Emission Spectra, H Lines, Stellar Activity, Stellar Spectra, Symbiotic Stars, Absorption Spectra, Metallicity, Radiant Flux Density, Stellar Envelopes

Scientific paper

Changes which took place in the CH Cyg emission line spectrum during
1978-1982 are studied. The yearly metal and hydrogen line intensities
are given. The behavior of hydrogen lines during 1979, when the shell
absorption spectrum began to form, is observed in detail.

Affiliated with

Also associated with

No associations

Rating

Spectral observations of CH Cyg. II - Emission lines from 1978 to 1982 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 Spectral observations of CH Cyg. II - Emission lines from 1978 to 1982, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral observations of CH Cyg. II - Emission lines from 1978 to 1982 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1125748