Why soft X-ray transients can remain in the low/hard state during outburst

Astronomy and Astrophysics

Volumn 423, Issue 1, 2004, Pages 321-326

  Meyer Hofmeister, E ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Accretion, accretion disks; Black hole physics; Stars: individual: GRO J0422; Stars: individual: XTE J1118+480; X rays: binaries

Indexed keywords

ACCREDITATION; EVAPORATION; GALAXIES; IONIZATION; MATHEMATICAL MODELS; PARAMETER ESTIMATION; RADIATION EFFECTS; X RAY ANALYSIS;

ACCRETION; LOW-MASS X-RAY BINARIES (LMXB); OUTBURST; X-RAY TRANSIENTS;

COSMIC RAYS;

EID: 4043100561     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040369     Document Type: Article

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