{ "id": "2203.06576", "version": "v1", "published": "2022-03-13T05:54:20.000Z", "updated": "2022-03-13T05:54:20.000Z", "title": "A global look into the world of interacting supernovae", "authors": [ "Anjasha Gangopadhyay", "Kuntal Misra", "Koji Kawabata", "Raya Dastidar", "Mridweeka Singh" ], "comment": "9 pages, 8 figures, Accepted for Special Issue of Journal of Astrophysics and Astronomy, 2022, Astrophysical jets and observational facilities: National perspective, 05 -09 April 2021, ARIES Nainital", "categories": [ "astro-ph.HE" ], "abstract": "Interacting supernovae (SNe) IIn and Ibn show narrow emission lines and have always been a mysterious and unsolved genre in SNe physics. We present a comprehensive analysis of the temporal and spectroscopic behaviour of a group of interacting SNe~IIn and Ibn. We choose SNe~2012ab, 2020cui, 2020rc and 2019uo as representative members of these SN sub-types to probe the nature of explosion. Our study reveals that SNe~IIn are heterogeneous, bright depicting multi-staged temporal evolution while SNe~Ibn are moreover homogeneous, comparatively fainter than SNe~IIn and short lived, but limited in sample to firmly constrain the homogeneity. The spectroscopic features display a great diversity in H$\\alpha$ and He profiles for both SNe~IIn and Ibn. The representative SN~Ibn also show flash ionisation signatures of CIII and NIII. Modelling of H$\\alpha$ reveals that SNe~IIn have in general an asymmetric CSM which interacts with SN ejecta resulting in diversity in H$\\alpha$ profiles.", "revisions": [ { "version": "v1", "updated": "2022-03-13T05:54:20.000Z" } ], "analyses": { "keywords": [ "interacting supernovae", "global look", "bright depicting multi-staged temporal evolution", "narrow emission lines", "spectroscopic features display" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }