A Novel Method of Modeling Extended Emission of Compact Jets: Application to Swift J1727.8−1613
Flat radio spectra of compact jets launched by both supermassive and stellar-mass black holes (BHs) are explained by an interplay of self-absorbed synchrotron emission up to some distance along the jet and optically thin synchrotron at larger distances. Their spatial structure is usually studied usi...
I tiakina i:
| Ngā kaituhi matua: | , , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2025-01-01
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| Rangatū: | The Astrophysical Journal Letters |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/2041-8213/ade13b |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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