Establishing the nature of companion candidates to X-ray-emitting late B-type stars

Monthly Notices of the Royal Astronomical Society

Volumn 381, Issue 4, 2007, Pages 1569-1574

  Hubrig, S ^a   Marco, O ^a   Stelzer, B ^b   Scholler M ^a   Huelamo N ^c  

^a EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

Author keywords

Binaries: spectroscopic; Binaries: visual; Stars: pre main sequence; X rays: stars

Indexed keywords

ADAPTIVE OPTICS; ELECTROMAGNETIC WAVE EMISSION; STARS;

BINARIES: SPECTROSCOPIC; BINARIES:VISUAL; LATE-TYPE; LATE-TYPE STARS; SPECTRAL TYPES; STARS: BE; STARS: PRE-MAIN SEQUENCE; X-RAY EMISSION; X-RAY EMITTING; X-RAY:STARS;

X RAY SCATTERING;

EID: 35748929384     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12325.x     Document Type: Article

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