<i>José Bonifacio cientista, professor e técnico</i>
            de Elysario Tavora Filho

Figueira, Gastón

doi:10.5195/reviberoamer.1947.1235

Cited by 1 publication

(1 citation statement)

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“…Very recent works on the subject are those by Gray et al (2016) and Boehner et al (2017). The collision of a typical nova ejecta with a main sequence companion star was recently studied by Figueira et al (2018), where the fate of the accretion disc surrounding the white dwarf was addressed.…”

Section: Spheres With the Sd Scenario Of Sne Iamentioning

confidence: 99%

Interaction of Hemispherical Blast Waves with Inhomogeneous Spheres: Probing the Collision of a Supernova Ejecta with a Nearby Companion Star in the Laboratory

Garcı́a-Senz

Velarde

Suzuki-Vidal

et al. 2019

ApJ

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Past high-energy density laboratory experiments provided insights into the physics of supernovae, supernova remnants, and the destruction of interstellar clouds. In a typical experimental setting, a laser-driven planar blast wave interacts with a compositionally-homogeneous spherical or cylindrical target. In this work we propose a new laboratory platform that accounts for curvature of the impacting shock and density stratification of the target. Both characteristics reflect the conditions expected to exist shortly after a supernova explosion in a close binary system.We provide details of a proposed experimental design (laser drive, target configuration, diagnostic system), optimized to capture the key properties of recent ejecta-companion interaction models. Good qualitative agreement found between our experimental models and their astrophysical counterparts highlights strong potential of the proposed design to probe details of the ejecta-companion interaction for broad classes of objects by means of high energy density laboratory experiments.

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Section: Spheres With the Sd Scenario Of Sne Iamentioning

confidence: 99%