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dc.date.accessioned | 2021-09-23T14:56:05Z | |
dc.date.available | 2021-09-23T14:56:05Z | |
dc.date.issued | 2021-04-13 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/125482 | |
dc.description.abstract | We present the photometric and spectroscopic evolution of supernova (SN) 2019cad during the first ∼100 d from explosion. Based on the light-curve morphology, we find that SN 2019cad resembles the double-peaked Type Ib/c SN 2005bf and the Type Ic PTF11mnb. Unlike those two objects, SN 2019cad also shows the initial peak in the redder bands. Inspection of the g-band light curve indicates the initial peak is reached in ∼8 d, while the r-band peak occurred ∼15 d post-explosion. A second and more prominent peak is reached in all bands at ∼45 d past explosion, followed by a fast decline from ∼60 d. During the first 30 d, the spectra of SN 2019cad show the typical features of a Type Ic SN, however, after 40 d, a blue continuum with prominent lines of Si II λ6355 and C II λ6580 is observed again. Comparing the bolometric light curve to hydrodynamical models, we find that SN 2019cad is consistent with a pre-SN mass of 11 M⊙, and an explosion energy of 3.5 × 10⁵¹ erg. The light-curve morphology can be reproduced either by a double-peaked ⁵6⁶Ni distribution with an external component of 0.041 M⊙, and an internal component of 0.3 M⊙ or a double-peaked ⁵⁶Ni distribution plus magnetar model (P ∼ 11 ms and B ∼ 26 × 10¹⁴ G). If SN 2019cad were to suffer from significant host reddening (which cannot be ruled out), the ⁵⁶Ni model would require extreme values, while the magnetar model would still be feasible. | en |
dc.format.extent | 4907-4922 | es |
dc.language | en | es |
dc.subject | Supernovae: general | es |
dc.subject | Supernovae: individual: SN 2019cad | es |
dc.title | The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object | en |
dc.type | Articulo | es |
sedici.identifier.other | arXiv:2104.03723 | es |
sedici.identifier.other | doi:10.1093/mnras/stab1009 | es |
sedici.identifier.issn | 0035-8711 | es |
sedici.identifier.issn | 1365-2966 | es |
sedici.creator.person | Bersten, Melina Cecilia | es |
sedici.creator.person | Ertini, Keila Yael | es |
sedici.creator.person | Folatelli, Gastón | es |
sedici.subject.materias | Ciencias Astronómicas | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Instituto de Astrofísica de La Plata | es |
sedici.subtype | Preprint | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.description.peerReview | peer-review | es |
sedici.relation.journalTitle | Monthly Notices of the Royal Astronomical Society | es |
sedici.relation.journalVolumeAndIssue | vol. 504, no. 4 | es |