On the 2011 outburst of the Recurrent Nova T Pyxidis
L. Izzo, M. Della Valle, A. Ederoclite, M. Henze
TL;DR
This paper analyzes the nebular phase emission and line profiles during the 2011 outburst of the recurrent nova T Pyxidis, providing insights into the system's properties and the white dwarf mass.
Contribution
It offers new preliminary analysis of nebular emission lines and discusses the binary system configuration and X-ray emission in T Pyxidis.
Findings
White dwarf mass likely exceeds 0.8 M⊙
Line profile analysis reveals nebular emission characteristics
Discussion on binary system configuration and X-ray emission
Abstract
We discuss the nebular phase emission during the 2011 outburst of the recurrent nova T Pyxidis and present preliminary results on the analysis of the line profiles. We also present some discussions about the binary system configurations and the X-ray emission, showing that the white dwarf mass should be larger than 0.8 M.
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Taxonomy
TopicsAstrophysical Phenomena and Observations · High-pressure geophysics and materials · X-ray Spectroscopy and Fluorescence Analysis