The recurrent nova WZ Sagittae

Details The recurrent nova WZ Sagittae The recurrent nova WZ Sagittae

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..938v&link_type=abstract

Astronomicheskii Zhurnal, Vol. 60, p.938

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Spectral observations have been carried out five months before and a
year and a half after the flare. The intensities of the wide absorption
lines and of the two-component hydrogen emission vary during the orbital
period. There are two ranges of phases when the two-component emission
structure disappears.

Affiliated with

Also associated with

No associations

Rating

The recurrent nova WZ Sagittae 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 The recurrent nova WZ Sagittae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The recurrent nova WZ Sagittae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1192826