scholarly journals ACCRETION FLOW DYNAMICS OF MAXI J1659-152 FROM THE SPECTRAL EVOLUTION STUDY OF ITS 2010 OUTBURST USING THE TCAF SOLUTION

2015 ◽  
Vol 803 (2) ◽  
pp. 59 ◽  
Author(s):  
Dipak Debnath ◽  
Aslam Ali Molla ◽  
Sandip K. Chakrabarti ◽  
Santanu Mondal
1997 ◽  
Vol 163 ◽  
pp. 824-825
Author(s):  
John C. L. Wang ◽  
Ralph S. Sutherland

The ~ 108−109 old neutron stars in the Galaxy may be undergoing low luminosity accretion from the interstellar medium (Ostriker et al. 1970; Shvartsman 1971). It was first recognized by Shvartsman (1971) that the accretion induced radiation from the stellar surface can heat the infalling material, which in turn inhibits further accretion. This preheating instability has been studied in detail in the high luminosity regime where equilibrium ionization and heating holds (e.g., Buff & McCray 1974; Ostriker et al. 1976; Cowie et al. 1978). In the low luminosity regime, however, dynamical timescales are typically much shorter than atomic timescales so the accretion flow dynamics is strongly coupled to non-equilibrium (NEQ) atomic processes (cf. Blaes et al. 1995).


2016 ◽  
Vol 831 (1) ◽  
pp. 4 ◽  
Author(s):  
Hung-Yi Pu ◽  
Kazunori Akiyama ◽  
Keiichi Asada

2016 ◽  
Vol 819 (2) ◽  
pp. 107 ◽  
Author(s):  
Arghajit Jana ◽  
Dipak Debnath ◽  
Sandip K. Chakrabarti ◽  
Santanu Mondal ◽  
Aslam Ali Molla
Keyword(s):  

2019 ◽  
Vol 882 (2) ◽  
pp. 82 ◽  
Author(s):  
Britton Jeter ◽  
Avery E. Broderick ◽  
B. R. McNamara

2018 ◽  
Vol 363 (5) ◽  
Author(s):  
Anuj Nandi ◽  
S. Mandal ◽  
H. Sreehari ◽  
D. Radhika ◽  
Santabrata Das ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document