Population X: Are the super-Eddington X-ray sources beamed jets in microblazars or intermediate mass black holes?

Astronomy and Astrophysics

Volumn 382, Issue 3, 2002, Pages

  Kording E ^a   Falcke, H ^a   Markoff, S ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Accretion, accretion disks; Black hole physics; Radiation mechanisms: non thermal; X rays: binaries

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; MATHEMATICAL MODELS; SPECTRUM ANALYSIS; SYNCHROTRON RADIATION; X RAY ANALYSIS;

ULTRA-LUMINOUS X-RAY SOURCES (ULX);

ASTROPHYSICS;

EID: 0036473047     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20011776     Document Type: Article

References (24)