Recovers the probability distribution of galaxy cluster 3-D shapes from single 2-D X-ray images using filamentarity, finding shape variation from prolate inner gas to oblate outer gas in 89 Chandra clusters.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.CO 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The probability distribution of 3-D shapes of galaxy clusters from 2-D X-ray images
Recovers the probability distribution of galaxy cluster 3-D shapes from single 2-D X-ray images using filamentarity, finding shape variation from prolate inner gas to oblate outer gas in 89 Chandra clusters.