Pregled bibliografske jedinice broj: 1029558
Linear spectropolarimetry of 35 Type Ia supernovae with VLT/FORS: an analysis of the Si II line polarization
Linear spectropolarimetry of 35 Type Ia supernovae with VLT/FORS: an analysis of the Si II line polarization // Monthly notices of the Royal Astronomical Society, 490 (2019), 1; 578-599 doi:10.1093/mnras/stz2322 (međunarodna recenzija, članak, znanstveni)
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Naslov
Linear spectropolarimetry of 35 Type Ia supernovae with VLT/FORS: an analysis of the Si II line polarization
Autori
Cikota, Aleksandar ; Patat, Ferdinando ; Wang, Lifan ; Wheeler, J. Craig ; Bulla, Mattia ; Baade, Dietrich ; Höflich, Peter ; Cikota, Stefan ; Clocchiatti, Alejandro ; Maund, Justyn R. ; Stevance, Heloise F. ; Yang, Yi
Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 490
(2019), 1;
578-599
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
supernovae ; polarization
Sažetak
Spectropolarimetry enables us to measure the geometry and chemical structure of the ejecta in supernova explosions, which is fundamental for the understanding of their explosion mechanism(s) and progenitor systems. We collected archival data of 35 Type Ia Supernovae (SNe Ia), observed with FORS on the Very Large Telescope at 127 epochs in total. We examined the polarization of the Si II λ6355 Å line (pSiII) as a function of time which is seen to peak at a range of various polarization degrees and epochs relative to maximum brightness. We reproduced the Δm15-pSiII relationship identified in a previous study, and show that subluminous and transitional objects display polarization values below the Δm15-pSiII relationship for normal SNe Ia. We found a statistically significant linear relationship between the polarization of the Si II λ6355 Å line before maximum brightness and the Si II line velocity and suggest that this, along with the Δm15-pSiII relationship, may be explained in the context of a delayed-detonation model. In contrast, we compared our observations to numerical predictions in the Δm15-vSiII plane and found a dichotomy in the polarization properties between Chandrasekhar and sub-Chandrasekhar mass explosions, which supports the possibility of two distinct explosion mechanisms. A subsample of SNe display evolution of loops in the q-u plane that suggests a more complex Si structure with depth. This insight, which could not be gleaned from total flux spectra, presents a new constraint on explosion models. Finally, we compared our statistical sample of the Si II polarization to quantitative predictions of the polarization levels for the double-detonation, delayed-detonation, and violent-merger models.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Fakultet elektrotehnike i računarstva, Zagreb
Profili:
Stefan Cikota
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus