A three-dimensional reconstruction of the interstellar magnetic field toward a star-forming region
Context. The polarized thermal emission from interstellar dust offers a valuable tool for probing both the dust and the magnetic field in the interstellar medium (ISM). However, existing observations only yield the total amount of dust emission along the line of sight (LoS), with no information on i...
Kaydedildi:
| Asıl Yazarlar: | , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
EDP Sciences
2026-01-01
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| Seri Bilgileri: | Astronomy & Astrophysics |
| Konular: | |
| Online Erişim: | https://www.aanda.org/articles/aa/full_html/2026/01/aa51034-24/aa51034-24.html |
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