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| SN 2020faa , the SIMBAD biblio (22 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST04:24:48 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
2021A&A...646A..22Y |
167 | T K A | D | X C | 3 | 5 | ~ |
Is supernova SN 2020faa an iPTF14hls look-alike? |
YANG S., SOLLERMAN J., CHEN T.-W., et al. |
| 2021MNRAS.504.5967S | 42 | X | 1 | 3 | ~ | Double common envelope jets supernovae (CEJSNe) by triple-star systems. | SOKER N. | ||
| 2021MNRAS.506.2445S | 42 | X | 1 | 5 | ~ | Binary neutron star merger in common envelope jets supernovae. | SOKER N. | ||
| 2021MNRAS.507.1651G | 51 | X | 1 | 3 | 27 | Common envelope jets supernovae with a black hole companion as possible high-energy neutrino sources. | GRICHENER A. and SOKER N. | ||
| 2021MNRAS.508.2386S | 42 | X | 1 | 6 | ~ | Simulating highly eccentric common envelope jet supernova impostors. | SCHREIER R., HILLEL S., SHIBER S., et al. | ||
| 2022MNRAS.509.2836S | 43 | X | 1 | 3 | ~ | Spin-orbit misalignment from triple-star common envelope evolution. | SOKER N. | ||
| 2022ApJ...926L..11S | 43 | X | 1 | 51 | 2 | Optical Rebrightening of Extragalactic Transients from the Zwicky Transient Facility. | SORAISAM M., MATHESON T., LEE C.-H., et al. | ||
| 2022ApJ...927..148C | 43 | X | 1 | 3 | ~ | A Physical Model of Delayed Rebrightenings in Shock-interacting Supernovae without Narrow-line Emission. | COUGHLIN E.R. and ZRAKE J. | ||
| 2022MNRAS.514.3212H | 88 | X | 2 | 5 | 18 | Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernovae. | HILLEL S., SCHREIER R. and SOKER N. | ||
| 2022RAA....22e5010S | 44 | X | 1 | 14 | 25 | A Common Envelope Jets Supernova (CEJSN) Impostor Scenario for Fast Blue Optical Transients. | SOKER N. | ||
| 2022ApJ...933..102W | 43 | X | 1 | 4 | 3 | iPTF14hls in the Circumstellar Medium Interaction Model: A Promising Candidate for a Pulsational Pair-instability Supernova. | WANG L.-J., LIU L.-D., LIN W.-L., et al. | ||
| 2022MNRAS.515.5473R | 43 | X | 1 | 5 | ~ | The response of a red supergiant to a common envelope jets supernova (CEJSN) impostor event. | RAGOLER N., BEAR E., SCHREIER R., et al. | ||
| 2022A&A...667A..92O | 102 | D | F | 2 | 25 | 2 | Supernova double-peaked light curves from double-nickel distribution. | ORELLANA M. and BERSTEN M.C. | |
|
2022ApJ...939..105B |
128 | S X | 2 | 121 | 10 | Seven Years of Coordinated Chandra-NuSTAR Observations of SN 2014C Unfold the Extreme Mass-loss History of Its Stellar Progenitor. | BRETHAUER D., MARGUTTI R., MILISAVLJEVIC D., et al. | ||
| 2022RAA....22l2003S | 43 | X | 1 | 54 | 19 | The Role of Jets in Exploding Supernovae and in Shaping their Remnants. | SOKER N. | ||
| 2023MNRAS.520.4182S | 45 | X | 1 | 5 | 6 | Simulating the deposition of angular momentum by jets in common envelope evolution. | SCHREIER R., HILLEL S. and SOKER N. | ||
| 2023MNRAS.522..885C | 44 | X | 1 | 5 | 1 | Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant. | COHEN T. and SOKER N. | ||
| 2023A&A...673A.127S | 4814 | T K A | S X C F | 107 | 11 | ~ |
Hidden shock powering the peak of SN 2020faa. |
SALMASO I., CAPPELLARO E., TARTAGLIA L., et al. | |
| 2024A&A...690A..17S | 3360 | K A | D | S X C | 74 | 12 | ~ | The story of SN 2021aatd: A peculiar 1987A-like supernova with an early-phase luminosity excess. | SZALAI T., KONYVES-TOTH R., NAGY A.P., et al. |
|
2025A&A...695A..29S |
93 | X | 2 | 36 | ~ | The diversity of strongly interacting Type IIn supernovae. | SALMASO I., CAPPELLARO E., TARTAGLIA L., et al. | ||
| 2025ApJ...992....9Z | 140 | X | 3 | 14 | ~ | SN 2019tsf: Evidence for Extended Hydrogen-poor CSM in the Three-peaked Light Curve of Stripped Envelope of a Type Ib Supernova. | ZENATI Y., WANG Q., BOBRICK A., et al. | ||
|
2025A&A...703A.177T |
47 | X | 1 | 31 | ~ | Signatures of anti-social mass loss in the ordinary Type II SN 2024bch A non-interacting supernova with early high-ionisation features. | TARTAGLIA L., VALERIN G., PASTORELLO A., et al. |