Reason for reduction of emission-line widths in the postmaximum spectrum of Nova Cygni 1975

Details Reason for reduction of emission-line widths in the postmaximum spectrum of Nova Cygni 1975 Reason for reduction of emission-line widths in the postmaximum spectrum of Nova Cygni 1975

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..226g&link_type=associated

Pis'ma v Astronomicheskii Zhurnal, vol. 3, May 1977, p. 226-228. In Russian.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Novae, Spectral Line Width, Stellar Spectra, Energy Dissipation, Kinetic Energy, Shock Heating, Stellar Envelopes

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

Reason for reduction of emission-line widths in the postmaximum spectrum of Nova Cygni 1975 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 Reason for reduction of emission-line widths in the postmaximum spectrum of Nova Cygni 1975, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Reason for reduction of emission-line widths in the postmaximum spectrum of Nova Cygni 1975 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1883448