Published June 22, 2021 | Version 0

The metal content of the hot atmospheres of galaxy groups - supporting data

  • 1. IASF – Milano
  • 2. SRON
  • 3. ESTEC
  • 4. INAF - Osservatorio Astronomico di Trieste,
  • 5. INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
  • 6. Saitama University
  • 7. Tokyo University of Science

Description

Supporting data used to generate the figures included in the review chapter "The metal content of the hot atmospheres of galaxy groups", to appear in the MDPI journal "Universe". These values were collected and compiled from existing literature; each text file lists the relevant references to the original articles where various sets of results were initially published. 

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data_for_Fig.4a.txt

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md5:af7b77532757c209a59f8cec39f5c941
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md5:1f86031ab2479032dcc859ffb7395a96
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md5:e1d325f5dd32832012c5f58e2697b73b
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Additional details

Related works

Is supplement to
Journal article: https://www.mdpi.com/2218-1997/7/7/208 (URL)