Pre-outburstChandraobservations of the recurrent nova T Pyxidis

2014/10/10 by Ş. Balman, Solen Balman · 2 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Laser-Plasma Interactions and Diagnostics #Nova (rocket) #Physics #astro-ph.HE

paper · pdf · doi:10.1051/0004-6361/201424233

published as A&A 572, A114 (2014) · 14 pages, 2 Tables, and 6 Figures, Astronomy and Astrophysics in Press

arxiv created 2014/10/10 · openalex publication_date 2014/10/15 · arxiv updated 2014/12/10 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. I study the spectral, temporal, and spatial characteristics of the quiescent X-ray emission (not in outburst) of the recurrent nova T Pyx.

Citations

• ChandraObservation of the Shell of Nova Persei 1901 (GK Persei): Detection of Localized Nonthermal X‐Ray Emission from a Miniature Supernova Remnant
• SwiftObservations of the 2006 Outburst of the Recurrent Nova RS Ophiuchi. I. Early X‐Ray Emission from the Shocked Ejecta and Red Giant Wind
• Two Types of X-Ray Spectra in Cataclysmic Variables
• Advection-dominated accretion and the black hole event horizon
• HIGH-RESOLUTION X-RAY SPECTROSCOPY OF THE EVOLVING SHOCK IN THE 2006 OUTBURST OF RS OPHIUCHI
• The 2011 outburst of the recurrent nova T Pyxidis. Evidence for a face-on bipolar ejection
• X-ray spectral variations of U Gem from quiescence to outburst
• The secrets of T Pyxidis

Cited by

• X-ray observations of the nova shell IPHASX J210204.7+471015
• Extended X-ray emission from the classic nova DQ Her – on the possible presence of a magnetized jet