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The Escape of Ionizing Photons from the Galaxy

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Bland-Hawthorn, J., Maloney, Philip R.·1999·The Astrophysical Journal

Abstract

The Magellanic Stream and several high-velocity clouds have now been detected in optical line emission. The observed emission measures and kinematics are most plausibly explained by photoionization due to hot, young stars in the Galactic disk. The highly favorable orientation of the Stream allows an unambiguous determination of the fraction of ionizing photons f which escape the Galactic disk. We have modeled the production and transport of ionizing photons through an opaque interstellar medium. Normalization to the Stream detections requires f ≈6%, which is in reasonable agreement with the flux required to ionize the Reynolds layer. Neither shock heating nor emission within a hot Galactic corona can be important in producing the observed Hα emission. If such a large escape fraction is typical of L galaxies, star-forming systems dominate the extragalactic ionizing background. Within the context of this model, both the three-dimensional orientation of the Stream and the distances to high-velocity clouds can be determined by sensitive Hα observations.

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Metadata

Authors
Bland-Hawthorn, J., & Maloney, P. R.
Venue
The Astrophysical Journal
Published
1999-01-01
Volume
510
Issue
1
Pages
L33-L36
ISSN
0004-637X (ISSN-L)
OpenAlex
W2073084722
Cited by
191
References
0
FWCI
14.34
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The Escape of Ionizing Photons from the Galaxy. https://app.cochat.ai/papers/10.1086/311797
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Bland-Hawthorn, J., & Maloney, P. R. (1999). The Escape of Ionizing Photons from the Galaxy. The Astrophysical Journal. https://doi.org/10.1086/311797

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