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

Monte Carlo simulations of the detailed iron absorption line profiles from thermal winds in X-ray binaries

Ryota Tomaru, Chris Done, Hirokazu Odaka, Shin Watanabe, Tadayuki Takahashi

Monthly Notices of the Royal Astronomical Society · 2018

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Summary

This paper is not relevant to Vitagri's Pulse Brain catalogue. It concerns X-ray binary astronomy—specifically the modelling of iron absorption line profiles in accretion disc winds around neutron stars—rather than farming systems, soil health, nutrient density, or human nutrition. The work applies Monte Carlo radiation transfer simulations to understand thermal wind dynamics in high-energy astrophysical systems, with no connection to agricultural or nutritional science.

UK applicability

Not applicable. This is an astrophysics study with no bearing on UK agricultural policy, land management, soil health, or nutritional outcomes.

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/sty336
Catalogue ID
BFmohg5fgd-fdxlvg

Topic tags

x-ray binariesaccretion discsiron absorption linesradiation transferneutron starsastrophysics
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