Can activity of the secondary component explain the emission-line spectra of cataclysmic binaries?

Details Can activity of the secondary component explain the emission-line spectra of cataclysmic binaries? Can activity of the secondary component explain the emission-line spectra of cataclysmic binaries?

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984obs...104..186r&link_type=abstract

The Observatory, vol. 104, p. 186-188 (1984)

Computer Science

1

Scientific paper

It is shown that the emission lines of C IV observed in cataclysmic
dwarf-nova binaries in quiescence cannot be due to the magnetic activity
of the secondary components; these stars are much too faint to provide
the necessary emission-line fluxes.

Affiliated with

Also associated with

No associations

Rating

Can activity of the secondary component explain the emission-line spectra of cataclysmic binaries? 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 Can activity of the secondary component explain the emission-line spectra of cataclysmic binaries?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Can activity of the secondary component explain the emission-line spectra of cataclysmic binaries? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1678140