File:2010jl-like supernovae.png
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Summary
| Description |
English: 2010jl-like supernovae with NEOWISE.
Data was downloaded from IRSA: table "NEOWISE-R Single Exposure (L1b) Source Table" and the brightness was shifted with a constant value, which is labelled in the table. https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-scan?mission=irsa&submit=Select&projshort=WISE These supernovae show a first brightness increase around day 0 and a second increase about 200-600 days after their discovery (black circles). The first increase is from the interaction of the supernova with the circumstellar medium (CSM) and a light echo. The second increase in brightness is attributed with the formation of new dust. The following supernovae are shown: SN 2010jl, SN 2014ab, SN 2017hcc, ASASSN -15ua, SN 2016eei, SN 2017ijn The following publications describe these as 2010jl-like: Bevan et al. 2020 https://ui.adsabs.harvard.edu/abs/2020ApJ...894..111B/abstract Moriya et al. 2020 https://ui.adsabs.harvard.edu/abs/2020A%26A...641A.148M/abstract Moran et al. 2023 https://ui.adsabs.harvard.edu/abs/2023A%26A...669A..51M/abstract Dickinson et al. 2024 https://ui.adsabs.harvard.edu/abs/2024MNRAS.527.7767D/abstract Thévenot 2020 https://ui.adsabs.harvard.edu/abs/2020RNAAS...4..243T/abstract |
| Date | |
| Source | Own work |
| Author | Meli thev |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:57, 1 February 2024 | | 792 × 712 (56 KB) | Meli thev | Uploaded own work with UploadWizard |
