Does the Milky Way launch a large-scale wind?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Ism: Outflows, Galaxy: Bulge, Galaxy: Dynamics, Galaxy: Evolution

Scientific paper

The ROSAT All-Sky Survey revealed soft X-ray emission on kiloparsec scales towards the Galactic center. Separately, it has also been observed that the cosmic ray intensity (measured via γ-ray emission) rises only very slowly towards the center of the Galaxy, counter to expectations based on the greater number of cosmic ray sources there. A thermal and cosmic-ray driven wind could potentially explain both of these observations. We find that a cosmic-ray and thermally driven wind fits the X-ray observations well; in fact, a wind fits significantly better than an earlier-proposed static-polytrope gas model.

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