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ZENODO
Conference object . 2019
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Conference object . 2019
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Other literature type . 2019
License: CC BY
Data sources: ZENODO
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Properties of the mass stream– accreting matter interaction in two Double White Dwarfs

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 12 Jul 2019Publisher:Zenodo
Authors: Boneva, Daniela; Boeva, Svetlana;

doi: 10.5281/zenodo.3333502 , 10.5281/zenodo.3333503

Properties of the mass stream– accreting matter interaction in two Double White Dwarfs

Abstract

We investigate the mass transfer properties at the evolutionary stage after the mass transfer being started, in two Double White Dwarfs binary stars – CR Boo and V 803 Cen. Both are AM CVn stars objects: short period binaries; helium-rich accreting material; The mass transfer is considered to be realized via the Roche-lobe overflow; Solutions of the mass transfer stability by the dynamical stability criteria; The accretion efficiency of two objects is estimated. The obtained values are very low.

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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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