Hydrodynamical Modelling of T Pyxidis

Details Hydrodynamical Modelling of T Pyxidis Hydrodynamical Modelling of T Pyxidis

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..252g&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

Stars: Supernovae, Stars: Individual (T Pyx)

Scientific paper

The Hubble Space Telescope observations showed that some nova outbursts may not produce smooth shells of gas, but thousands of gaseous blobs. In the case of T Pyx the blobs are distributed in eight concentric circles around the exploding star, producing a pattern similar to tree rings. We explore here the formation of the tree rings by hydrodynamical simulations.

Affiliated with

Also associated with

No associations

Rating

Hydrodynamical Modelling of T Pyxidis 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 Hydrodynamical Modelling of T Pyxidis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydrodynamical Modelling of T Pyxidis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-772100