Constraints on the Properties of Warm Ionized Gas from Low-frequency Hydrogen Radio Recombination Lines
The ionized gas in the Milky Way is a major component of the interstellar medium. Observations of extinction-free tracers, such as hydrogen radio recombination lines (HRRLs), have revealed the presence of a dense (electron density = 1–100 cm ^−3 ) warm ionized medium. Motivated by advances in radio...
Kaydedildi:
| Asıl Yazarlar: | , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2026-01-01
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| Seri Bilgileri: | The Astronomical Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/1538-3881/ae7a69 |
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