Pulse Brain · Growing Health Evidence Index
Tier 3 — Observational / field trialPeer-reviewed

The thermal-radiative wind in low-mass X-ray binary H1743−322: radiation hydrodynamic simulations

Ryota Tomaru, Chris Done, Ken Ohsuga, Mariko Nomura, Tadayuki Takahashi

Monthly Notices of the Royal Astronomical Society · 2019

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Summary

This paper is an astrophysical study of accretion disc winds in a black hole X-ray binary system (H1743−322) using radiation hydrodynamic simulations. The work models thermal-radiative wind dynamics and is not relevant to agricultural, soil health, nutrient density, or human nutrition research.

UK applicability

This astrophysics paper has no applicability to UK farming systems, soil health, nutrient density, or human health research and falls outside Vitagri's Pulse Brain scope.

Theme
General food systems / other
Subject
Other / interdisciplinary
Study type
Research
Study design
Research
Source type
Peer-reviewed study
Status
Published
System type
Other
DOI
10.1093/mnras/stz2738
Catalogue ID
BFmobgho5x-fvrlzd

Topic tags

astrophysicsx-ray binaryaccretion discsradiation hydrodynamicsnot-food-systems
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