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Hydrodynamical Modelling of T Pyxidis

Published online by Cambridge University Press:  22 February 2018

Guillermo García-Segura ,
Mordecai-Mark Mac Low  and
Michael M. Shara
Guillermo García-Segura
Affiliation:
Instituto de Astronomía-UNAM
Mordecai-Mark Mac Low
Affiliation:
American Museum of Natural History
Michael M. Shara
Affiliation:
American Museum of Natural History

Extract

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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.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 252
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Dalgarno, A. & McCray, R. A. 1972, ARAA, 10, 375 Google Scholar
MacDonald, J. & Bailey, M. E. 1981, MNRAS, 197, 995 Google Scholar
Raymond, J. С. & Smith, B. W. 1977, ApJS, 35, 419 CrossRefGoogle Scholar
Shara, et al. 1997, AJ, 114, 258 Google Scholar
Stone, J. M. & Norman, M. L. 1992, ApJS, 80, 753 CrossRefGoogle Scholar