Evolution of the symbiotic nova RX Puppis
Abstract
We present and discuss a hundred year history of activity of the hot component of RX Pup based on optical photometry and spectroscopy. The outburst evolution of RX Pup resembles that of other symbiotic novae whereas at quiescence the hot component shows activity (high and low activity states) resembling that of symbiotic recurrent novae T CrB and RS Oph.
- Publication:
-
Classical Nova Explosions
- Pub Date:
- November 2002
- DOI:
- 10.1063/1.1518175
- arXiv:
- arXiv:astro-ph/0210505
- Bibcode:
- 2002AIPC..637...42M
- Keywords:
-
- 97.30.Qt;
- 97.80.Gm;
- 97.10.Cv;
- Novae dwarf novae recurrent novae and other cataclysmic variables;
- Cataclysmic binaries;
- symbiotic stars;
- Stellar structure interiors evolution nucleosynthesis ages;
- Astrophysics
- E-Print:
- To appear in in M. Hernanz, J. Jose, eds, Classical Novae Explosions, AIP