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ZENODO
Conference object . 2019
License: CC BY
Data sources: Datacite
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ZENODO
Other literature type . 2019
License: CC BY
Data sources: ZENODO
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ZENODO
Conference object . 2019
License: CC BY
Data sources: Datacite
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Formation of Close Double White Dwarfs: model results VS observation

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 01 Jul 2019Publisher:Zenodo
Authors: LI Huaju;

doi: 10.5281/zenodo.3265208 , 10.5281/zenodo.3265207

Formation of Close Double White Dwarfs: model results VS observation

Abstract

We do a binary population synthesis (BPS) simulation about the close double white dwarfs (CDWDs), two main BPS modifications are as follows. 1.The mass–orbital period relation after stable RLOF is implemented into our BPS code; 2.The mass transfer stability criterionis obtained from adiabatic mass loss model(Ge, H et al. 2015).

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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