The compact circumstellar material of SN 2024ggi: another supernova with a pre-explosion effervescent zone and jet-driven explosion
I examine recent theoretical studies and observations of the recent core-collapse supernova (CCSN) SN~20224ggi and find that the likely explanation for its dense, compact circumstellar material is an effervescent model, where parcels or streams of gas are uplifted by stellar convection and pulsation...
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| Μορφή: | Άρθρο |
| Γλώσσα: | English |
| Έκδοση: |
Maynooth Academic Publishing
2024-08-01
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| Σειρά: | The Open Journal of Astrophysics |
| Διαθέσιμο Online: | https://doi.org/10.33232/001c.122844 |