The origin of the supersoft X-ray-optical/UV flux anticorrelation in the symbiotic binary AG draconis

Astronomy and Astrophysics

Volumn 507, Issue 3, 2009, Pages 1531-1539

  Skopal, A ^a   Sekeras M ^a   Gonzalez Riestra R ^b   Viotti, R F ^c  

^a ASTRONOMICAL INSTITUTE   (Slovakia)

^b EUROPEAN SPACE AGENCY   (Spain)

^c INAF IASF ROMA   (Italy)

Author keywords

AG Draconis; Stars: binaries; Stars: fundamental parameters; Symbiotic; X rays: binaries; X rays: individuals

Indexed keywords

ANTICORRELATION; HIGH ENERGY PHOTONS; HIGH RESOLUTION; NEAR-IR; OPTICAL BURSTS; PARTICLE DENSITIES; SPECTRAL ENERGY DISTRIBUTION; STAR WINDS; STARS: BINARIES; STARS:FUNDAMENTAL PARAMETERS; UV SPECTROSCOPY; WHITE DWARFS; X-RAY EMISSION; X-RAYS: BINARIES; X-RAYS: INDIVIDUAL; XMM-NEWTON;

ELECTRIC POWER DISTRIBUTION; ELECTROMAGNETIC WAVE EMISSION; ELECTRON ENERGY LOSS SPECTROSCOPY; HELIUM; ION BEAMS; STARS; ULTRAVIOLET SPECTROSCOPY; WIND POWER; X RAY SCATTERING;

X RAYS;

EID: 70849112940     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811418     Document Type: Article

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