The secrets of T Pyx: I. UV observations

Abstract

We have studied the UV spectral behavior of the recurrent nova T Pyx during 16 years of IUE observations. We examined both the IUE line-by-line images and the extracted spectra in order to understand the reality and the origin of the observed spectral variations. The UV continuum of T Pyx has remained nearly constant in slope and intensity over this time interval, without any indication of long-term trends. The reddening determined from the UV data is E(B-V}=0.25 \pm 0.02. The best single-curve fit to the dereddened UV continuum is a power-law distribution $\propto {\lambda }^{-2.33}$. The tail of this curve agrees well with the B, V, and J magnitudes of T Pyx, indicating that the contribution of the secondary star is negligible. One peculiar aspect of T Pyx is that most emission lines (the strongest ones being those of CIV 1550 and HeII 1640) show substantial changes both in intensity and detectability, in contrast to the near constancy of the continuum. Several individual spectra display emission features that are difficult to identify, suggesting a composite spectroscopic system. We tentatively ascribe the origin of these transient emission features either to loops and jets from the irradiated secondary or to moving knots of the surrounding nebula that are (temporarily) projected in front of the system. The inspection of all IUE line-by-line images has led to the detection of emission spikes outside the central strip of the spectrum, which in some cases seem associated to known emission features in the (main) spectrum. A comparison with other ex-novae reveals a surprising similarity to the spectrum of the very-slow nova HR Del, whose white dwarf primary has a mass that is allegedly about one half that of T Pyx.

arXiv commentAccepted for publication in Astronomy and Astrophysics, Main Journal. 12 pages, 9 Figures

References in corpus (7)

• Detailed Mid- and Far-Ultraviolet Model Spectra for Accretion Disks in Cataclysmic Binaries
• The massive stellar content in NGC604 and its evolutionary state
• The INES System IV: The IUE Absolute Flux Scale
• T Pyxidis: The First Cataclysmic Variable with a Collimated Jet
• On the existence of jets in the recurrent nova T Pyxidis
• The Active Quiescence of HR Del (Nova Del 1967)
• Complex Velocity Fields in the Shell of T Pyxidis

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• The 2011 Outburst of Recurrent Nova T Pyx: X-ray Observations Expose the White Dwarf Mass and Ejection Dynamics
• A New Catalogue of Galactic Novae: Investigation of the MMRD relation & Spatial Distribution
• T Pyxidis: Death by a Thousand Novae
• The Distances of the Galactic Novae
• Optical observations of "hot" novae returning to quiescence
• SALT observations of southern post-novae
• Hubble Space Telescope Far Ultraviolet Spectroscopy of the Recurrent Nova T Pyxidis
• The Long-Term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis
• The XMM-Newton Detection of Extended Emission from the Nova Remnant of T Pyxidis
• Pre-outburst $Chandra$ Observations of the Recurrent Nova T Pyxidis
• The physical properties of T Pyx as measured by MUSE I. The geometrical distribution of the ejecta and the distance to the remnant