Probing the hot circumgalactic medium of external galaxies in X-ray absorption II: a luminous spiral galaxy at z ≈ 0.225
ABSTRACT The circumgalactic medium (CGM) is the most massive baryonic component of a spiral galaxy, shock heated to about 106 K for an $\rm L^{\star }$ galaxy. The CGM of the Milky Way has been well-characterized through X-ray absorption line spectroscopy. However, the paucity of bright background s...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society. Letters 2023-10, Vol.525 (1), p.L11-L16 |
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| Format: | Artikel |
| Sprache: | eng |
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