Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission

Astronomy and Astrophysics

Volumn 493, Issue 3, 2009, Pages 1049-1059

  Orlando, S ^a,b   Drake, J J ^c   Laming, J M ^d  

^a INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^b Consorzio COMETA ^*  (Italy)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d NAVAL RESEARCH LABORATORY   (United States)

Author keywords

Shock waves; Stars: Binaries: Symbiotic; Stars: Individual: RS Oph; Stars: Novae, cataclysmic variables; X rays: Binaries

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; EXPLOSIVES; FLUID DYNAMICS; HYDRODYNAMICS; ION BEAMS; RAPID SOLIDIFICATION; SHOCK WAVES; STARS; THREE DIMENSIONAL; X RAY SCATTERING; X RAYS;

ASPHERICAL; BLAST WAVES; BLUE-SHIFTED; CIRCUMSTELLAR; DENSITY ENHANCEMENTS; EMISSION LINES; FLUX SATURATIONS; HIGH QUALITY DATUM; HYDRODYNAMIC MODELING; HYDRODYNAMIC SIMULATIONS; LINE OF SIGHTS; LINE PROFILES; PLASMA TEMPERATURES; RADIATIVE COOLING; RED-SHIFTED EMISSIONS; SMALL REGIONS; STARS: BINARIES: SYMBIOTIC; STARS: INDIVIDUAL: RS OPH; STARS: NOVAE, CATACLYSMIC VARIABLES; THERMAL CONDUCTIONS; THREE-DIMENSIONAL MODELING; X-RAY ABSORPTIONS; X-RAY BANDS; X-RAY EMISSIONS; X-RAYS: BINARIES;

EMISSION SPECTROSCOPY;

EID: 59049098283     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810109     Document Type: Article

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