Radio and γ-ray Evidence for the Supernova Origin of High-velocity Cloud Complex M
Using λ 21 cm galactic neutral hydrogen data from the HI4PI survey and 0.75–30 MeV γ -ray emission from the Imaging Compton Telescope, we have searched for the origin event that accelerated high-velocity cloud Complex M. Radio plots of l − b , l − v , and b − v show a cavity centered at ( l , b ) ∼...
I tiakina i:
| Ngā kaituhi matua: | , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2023-01-01
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| Rangatū: | The Astrophysical Journal |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-4357/acae82 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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