Spectrophotometry of Nova Coronae Austrinae, 1981

Details Spectrophotometry of Nova Coronae Austrinae, 1981 Spectrophotometry of Nova Coronae Austrinae, 1981

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..163s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 1, Sept. 1984, p. 163-168.

Astronomy and Astrophysics

Astrophysics

1

Novae, Spectrum Analysis, Stellar Spectrophotometry, Black Body Radiation, Electron Density (Concentration), Emission Spectra, Hydrogen Ions, Ion Density (Concentration), Line Spectra, Stellar Envelopes

Scientific paper

Spectrophotometric observations of Nova Coronae Austrinae 1981, during
its nebular phase are reported. The various emission lines are
identified. The electron densities and the mass of the ionized hydrogen
in the shell have been calculated. The excess flux in the red continuum
probably indicates the appearance of the dust component.

Affiliated with

Also associated with

No associations

Rating

Spectrophotometry of Nova Coronae Austrinae, 1981 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 Spectrophotometry of Nova Coronae Austrinae, 1981, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of Nova Coronae Austrinae, 1981 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1390049