Pre-outburst Chandra observations of the recurrent nova T Pyxidis

BALMAN Ş.

ASTRONOMY & ASTROPHYSICS, vol.572, 2014 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 572
  • Publication Date: 2014
  • Doi Number: 10.1051/0004-6361/201424233
  • Journal Name: ASTRONOMY & ASTROPHYSICS
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Keywords: accretion, accretion disks, radiation mechanisms: thermal, stars: individual: T Pyxidis, novae, cataclysmic variables, binaries: close, X-rays: binaries, X-RAY-EMISSION, CLASSICAL NOVA, WHITE-DWARF, XMM-NEWTON, CATACLYSMIC VARIABLES, CONTINUUM EMISSION, SWIFT OBSERVATIONS, ACCRETION DISKS, ORBITAL PERIOD, BOUNDARY-LAYER
  • Istanbul University Affiliated: No

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.