A Disk Instability Interpretation for the 2001 Outburst of WZ SGE

Details A Disk Instability Interpretation for the 2001 Outburst of WZ SGE A Disk Instability Interpretation for the 2001 Outburst of WZ SGE

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..134o&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

Accretion, Accretion Disks, Binaries: Close, Stars: Dwarf Novae, Stars: Individual (Wz Sge)

Scientific paper

The 2001 outburst of WZ SGE is discussed based on the thermal-tidal
instability model (TTI model). It is demonstrated that the overall
development of the outburst can be understood by the disk instability
model (TTI model) and that no enhanced mass transfer is needed to
explain observations.

Affiliated with

Also associated with

No associations

Rating

A Disk Instability Interpretation for the 2001 Outburst of WZ SGE 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 A Disk Instability Interpretation for the 2001 Outburst of WZ SGE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Disk Instability Interpretation for the 2001 Outburst of WZ SGE will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-771902