Flaring Activity from Quiescent States in Neutron-Star X-Ray Binaries

Christodoulou, Dimitris M ; Laycock, Silas G T ; Kazanas, Demosthenes ; Contopoulos, Ioannis

关键词: ACCRETION DISKS;    BINARY STARS;    CYCLOTRONS;    MAGNETIC FIELDS;    NEUTRON STARS;    PULSARS;    STELLAR FLARES;    STELLAR LUMINOSITY;    STELLAR MASS ACCRETION;    X RAY BINARIES;   

RP-ID  :  GSFC-E-DAA-TN67186

学科分类：天体物理学

美国|英语

来源: NASA Technical Reports Server

【 摘 要 】

We examine systematically the observed X-ray luminosity jumps (or flares) from quiescent states in millisecond binary pulsars (MSBPs) and high-mass X-ray binary pulsars (HMXBPs). We rely on the published X-ray light curves of seven pulsars: four HMXBPs, two MSBPs and the ultraluminous X-ray pulsar M82 X-2. We discuss the physics of their flaring activities or lack thereof, paying special attention to their emission properties when they are found on the propeller line, inside the Corbet gap or near the light-cylinder barrier.We provide guiding principles for future interpretations of faint X-ray observations, as well as a method of constraining the propeller lines and the dipolar surfacemagnetic fields of pulsars using a variety of quiescent states. In the process, we clarify some disturbing inaccuracies that have made their way into the published literature.