High mass X-ray binaries in the LMC: Dependence on the stellar population age and the "propeller" effect

Astronomy and Astrophysics

Volumn 431, Issue 2, 2005, Pages 597-614

  Shtykovskiy, P ^a   Gilfanov, M ^a,b  

^a Russian Academy of Sciences   (Russian Federation)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Galaxies: Magellanic Clouds; Stars: neutron; X rays: binaries; X rays: galaxies

Indexed keywords

ASTRONOMY; DATA REDUCTION; EXTRAPOLATION; GALAXIES; OBSERVATORIES; SOLAR SYSTEM;

GALAXIES:MAGELLANIC CLOUDS; STARS:NEUTRON; SURFACE DENSITY; X-RAYS:BINARIES; X-RAYS:GALAXIES;

X RAYS;

EID: 13944268869     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041074     Document Type: Article

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