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Movie from QED I paper #928

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261e7a9
add movie for R8
aditivijayan Jan 29, 2025
d99421c
adding all runs
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adding all runs
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add zoom ins
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fix latex
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one more latex issue
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add section for Gallery
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is this how new line works?
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is this how new line works?
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is this how new line works?
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is this how new line works?
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add QED subsec
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add latex and fix typos
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Put "Simulation gallery" at the top of the nav menu
BenWibking Jan 30, 2025
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Update gallery.md
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11 changes: 10 additions & 1 deletion docs/docs/gallery.md
Original file line number Diff line number Diff line change
Expand Up @@ -2,7 +2,9 @@

## QED III

QED is a suite of simulations following supernova-driven outflows in varying galactic environments. The simulations follow outflows from a $1$ kpc$^2$ patch of galaxy up to a vertical height of $\sim$ few kpc in three galactic environments: Solar neighbourhood, inner, and outer galaxy.

QED is a suite of 3D hydrodynamic simulations which follow supernova-driven outflows in varying galactic environments. The QED follows outflows from a $1$ kpc$^2$ patch of galaxy up to a vertical height of $\sim$ few kpc. In the third of a series of QED papers, [found here](https://ui.adsabs.harvard.edu/abs/2025arXiv250200929V/abstract), we explore how outflow properties of the outflows depend on three galactic environments: Solar neighbourhood, inner, and outer galaxy.


### Solar Neighbourhood

Expand Down Expand Up @@ -57,3 +59,10 @@ In the Inner galaxy, the zoom-in shows how the disc seems to be breathing in and

<div style="padding:56.25% 0 0 0;position:relative;"><iframe src="https://player.vimeo.com/video/1051358716?badge=0&amp;autopause=0&amp;player_id=0&amp;app_id=58479" frameborder="0" allow="autoplay; fullscreen; picture-in-picture; clipboard-write; encrypted-media" style="position:absolute;top:0;left:0;width:100%;height:100%;" title="QED III - zoomed in Inner Galaxy"></iframe></div><script src="https://player.vimeo.com/api/player.js"></script>
<br />


### QED I

The first QED paper, [link here](https://ui.adsabs.harvard.edu/abs/2024MNRAS.52710095V/abstract), focuses on the metal loading properties of galactic winds launched from the Solar Neighbourhood. Initially, the galaxy is metal-free. As supernovae feedback launches outflows from the galaxy, the multiphase outflows are loaded differentially with metals. The hot phase carries most of the metals while the cooler gas, which is entrained from the disc, is metal-poor. The following movie shows midplane slices of density (top), oxygen mass density (middle), and metallicity (bottom).

<div style="padding:56.25% 0 0 0;position:relative;"><iframe src="https://player.vimeo.com/video/1052834630?h=ac2488dffe&amp;badge=0&amp;autopause=0&amp;player_id=0&amp;app_id=58479" frameborder="0" allow="autoplay; fullscreen; picture-in-picture; clipboard-write; encrypted-media" style="position:absolute;top:0;left:0;width:100%;height:100%;" title="QED I"></iframe></div><script src="https://player.vimeo.com/api/player.js"></script>
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