I What is a typical mass density for inter-galactic gas in a cluster?

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The typical mass density for inter-galactic gas in a cluster is approximately 1 atom per cubic meter, as derived from X-ray emission detections, particularly illustrated by the bullet cluster images. The discussion highlights the importance of using precise search terms, as many results focus on electron density rather than mass density. The participant expresses gratitude for the clarification and acknowledges the need for better search strategies. Overall, the conversation emphasizes the challenges in finding specific scientific data and the value of accurate terminology in research. Understanding inter-galactic gas density is crucial for astrophysical studies.
timjdoom
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As far as I'm aware, galaxy clusters typically have some level of hot gas permeating the entire cluster, which the galaxies within these cluster orbit each other within. What is the typical mass density of that gas?
I assume we can work it out from X-ray emission detections, such as shown with the famous bullet cluster images.
 
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OMG, thank you. I tried searching for "mass density of galaxy cluster gas" and variations but never intergalactic gas. The results I found focused on electron density and I struggled to understand the papers e.g. https://academic.oup.com/mnras/article/457/1/281/989241

Clearly I need google my exact question before posting it. Thank you again!
 
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"Pop III stars are thought to be composed entirely of helium and hydrogen with trace amounts of lithium, the ingredients left over after the Big Bang. They formed early on, around 200 million years after the universe began. These stars are extremely rare because they died out long ago, although scientists have hoped that the faint light from these distant, ancient objects would be detectable. Previous Population III candidates have been ruled out because they didn't meet the three main...

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