The Problem of the Flickering Activity of the Recurrent Nova T CrB

Details The Problem of the Flickering Activity of the Recurrent Nova T CrB The Problem of the Flickering Activity of the Recurrent Nova T CrB

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..328h&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 3

Other

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Cataclysmic Binaries, Symbiotic Stars, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

On the basis of our previous paper (Hric et al. 1998) we can proclaim that the existence of two emission-line regions can remarkably affect the flickering activity in the binary system. We could expect flickering activity dependence on the orbital phase. Deriving the energy of the flickering and comparing the derived value with the energy particularly needed for three possible areas where the source of the flickering could be settled down, we found the most plausible area to be in the unstable accretion onto the white dwarf, i.e. the boundary layer.

Affiliated with

Also associated with

No associations

Rating

The Problem of the Flickering Activity of the Recurrent Nova T CrB 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 Problem of the Flickering Activity of the Recurrent Nova T CrB, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Problem of the Flickering Activity of the Recurrent Nova T CrB will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-734954