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

The thermal-radiative wind in low-mass X-ray binary H1743−322 – II. Iron line predictions from Monte Carlo radiation transfer

Ryota Tomaru, Chris Done, Ken Ohsuga, Hirokazu Odaka, Tadayuki Takahashi

Monthly Notices of the Royal Astronomical Society · 2020

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Summary

This paper is not relevant to Vitagri's Pulse Brain catalogue. It presents astrophysical simulations of thermal-radiative winds in a low-mass X-ray binary black hole system (H1743−322), using Monte Carlo radiation transfer modelling to predict iron line absorption and emission features. The work has no connection to farming systems, soil health, nutrient density, food production, or human nutrition.

UK applicability

Not applicable. This is fundamental astrophysics research concerning accretion disc physics around black holes, with no relevance to UK agricultural practice, food systems, or public health policy.

Theme
General food systems / other
Subject
Other / interdisciplinary
Study type
Research
Study design
Laboratory / in vitro
Source type
Peer-reviewed study
Status
Published
System type
Other
DOI
10.1093/mnras/staa961
Catalogue ID
BFmohg5fgd-a92pfs

Topic tags

astrophysicsx-ray binariesradiation transferaccretion discs
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