Spectropolarimetry of Type II supernovae: II. Intrinsic supernova polarization and its relation to photometric and spectroscopic properties

dc.contributor.authorNagao T.
dc.contributor.authorPatat F.
dc.contributor.authorCikota A.
dc.contributor.authorBaade D.
dc.contributor.authorMattila S.
dc.contributor.authorKotak R.
dc.contributor.authorKuncarayakti H.
dc.contributor.authorBulla M.
dc.contributor.authorAyala B.
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id380638299
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/380638299
dc.date.accessioned2025-08-27T21:36:06Z
dc.date.available2025-08-27T21:36:06Z
dc.description.abstract<p> The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. The recent discovery of several highly aspherical core-collapse SNe is significant, and studying these is regarded as being crucial in order to understand the underlying explosion mechanism. Here, we study the intrinsic polarization of 15 hydrogen-rich core-collapse SNe and explore the relation between polarization and the photometric and spectroscopic properties of these objects. Our sample shows diverse properties of the continuum polarization. Most SNe show a low degree of polarization at early phases but a sudden rise to ∼1% at certain points during the photospheric phase followed by a slow decline during the tail phase, with a constant polarization angle. The variation in the timing of peak polarization values implies diversity in the explosion geometry: some SNe have aspherical structures only in their helium cores, while in other SNe such structures reach out to a significant part of the outer hydrogen envelope with a common axis from the helium core to the hydrogen envelope. Other SNe show high polarization from early phases and a change in polarization angle around the middle of the photospheric phase. This implies that the ejecta are significantly aspherical out to the outermost layer and have multi-directional aspherical structures. Exceptionally, the Type IIL SN 2017ahn shows low polarization at both the photospheric and tail phases. Our results show that the timing of the polarization rise in Type IIP SNe is likely correlated with their brightness, velocity, and the amount of radioactive Ni produced: brighter SNe with faster ejecta velocity and a larger <sup>56</sup>Ni mass have more extended aspherical explosion geometries. In particular, there is a clear correlation between the timing of the polarization rise and the explosion energy; that is, the explosion asphericity is proportional to the explosion energy. This implies that the development of a global aspherical structure, such as a jet, might be the key for the realisation of an energetic SN in the mechanism of SN explosions. <br></p>
dc.identifier.eissn1432-0746
dc.identifier.jour-issn0004-6361
dc.identifier.olddbid200712
dc.identifier.oldhandle10024/183739
dc.identifier.urihttps://www.utupub.fi/handle/11111/46762
dc.identifier.urlhttps://www.aanda.org/articles/aa/full_html/2024/01/aa46715-23/aa46715-23.html
dc.identifier.urnURN:NBN:fi-fe2025082785094
dc.language.isoen
dc.okm.affiliatedauthorNagao, Takashi
dc.okm.affiliatedauthorMattila, Seppo
dc.okm.affiliatedauthorKotak, Rubina
dc.okm.affiliatedauthorKuncarayakti, Hanindyo
dc.okm.affiliatedauthorDataimport, Suomen ESO-keskus
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherEDP Sciences
dc.publisher.countryFranceen_GB
dc.publisher.countryRanskafi_FI
dc.publisher.country-codeFR
dc.relation.articlenumberA11
dc.relation.doi10.1051/0004-6361/202346715
dc.relation.ispartofjournalAstronomy and Astrophysics
dc.relation.volume681
dc.source.identifierhttps://www.utupub.fi/handle/10024/183739
dc.titleSpectropolarimetry of Type II supernovae: II. Intrinsic supernova polarization and its relation to photometric and spectroscopic properties
dc.year.issued2024

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