The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object
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 sh...
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| Autores principales: | , , |
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| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/125482 |
| Aporte de: |
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I19-R120-10915-125482 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Ciencias Astronómicas Supernovae: general Supernovae: individual: SN 2019cad |
| spellingShingle |
Ciencias Astronómicas Supernovae: general Supernovae: individual: SN 2019cad Bersten, Melina Cecilia Ertini, Keila Yael Folatelli, Gastón The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object |
| topic_facet |
Ciencias Astronómicas Supernovae: general Supernovae: individual: SN 2019cad |
| description |
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. |
| format |
Articulo Preprint |
| author |
Bersten, Melina Cecilia Ertini, Keila Yael Folatelli, Gastón |
| author_facet |
Bersten, Melina Cecilia Ertini, Keila Yael Folatelli, Gastón |
| author_sort |
Bersten, Melina Cecilia |
| title |
The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object |
| title_short |
The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object |
| title_full |
The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object |
| title_fullStr |
The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object |
| title_full_unstemmed |
The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object |
| title_sort |
double-peaked type ic supernova 2019cad: another sn 2005bf-like object |
| publishDate |
2021 |
| url |
http://sedici.unlp.edu.ar/handle/10915/125482 |
| work_keys_str_mv |
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Repositorios |
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1764820451744284675 |