Fig. 4: Summary of three possible C IV CGM models. | Nature

Fig. 4: Summary of three possible C IV CGM models.

From: Observations of a Magellanic Corona

Fig. 4

Our three possible models for C IV in a LMC corona (a), interfaces with a LMC corona (b), interfaces with a Milky Way (MW) corona (c). Cartoon renditions show approximately 104 K, approximately 105 K, approximately 105.5 K and approximately 106K gas in blue, orange, yellow and pink hues, respectively. The dashed green line outlines model b, which best explains our observations.

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