Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/29324
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Dastidar, Raya | en_US |
dc.contributor.author | Misra, Kuntal | en_US |
dc.contributor.author | Singh, Mridweeka | en_US |
dc.contributor.author | Sahu, D. K. | en_US |
dc.contributor.author | Pastorello, A. | en_US |
dc.contributor.author | Gangopadhyay, Anjasha | en_US |
dc.contributor.author | TOMASELLA, Lina | en_US |
dc.contributor.author | BENETTI, Stefano | en_US |
dc.contributor.author | Terreran, G. | en_US |
dc.contributor.author | Sanwal, Pankaj | en_US |
dc.contributor.author | Kumar, Brijesh | en_US |
dc.contributor.author | Singh, Avinash | en_US |
dc.contributor.author | Kumar, Brajesh | en_US |
dc.contributor.author | Anupama, G. C. | en_US |
dc.contributor.author | Pandey, S. B. | en_US |
dc.date.accessioned | 2020-12-30T08:57:27Z | - |
dc.date.available | 2020-12-30T08:57:27Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29324 | - |
dc.description.abstract | We present photometry, polarimetry, and spectroscopy of the Type II supernova ASASSN-16ab/SN 2016B in PGC 037392. The photometric and spectroscopic follow-up commenced about 2 weeks after shock breakout and continued until nearly 6 months. The light curve of SN 2016B exhibits intermediate properties between those of Type IIP and IIL. The early decline is steep (1.68 ± 0.10 mag 100 d<SUP>-1</SUP>), followed by a shallower plateau phase (0.47 ± 0.24 mag 100 d<SUP>-1</SUP>). The optically thick phase lasts for 118 d, similar to Type IIP. The <SUP>56</SUP>Ni mass estimated from the radioactive tail of the bolometric light curve is 0.082 ± 0.019 M<SUB>☉</SUB>. High-velocity component contributing to the absorption trough of H α and H β in the photospheric spectra are identified from the spectral modelling from about 57-97 d after the outburst, suggesting a possible SN ejecta and circumstellar material interaction. Such high-velocity features are common in the spectra of Type IIL supernovae. By modelling the true bolometric light curve of SN 2016B, we estimated a total ejected mass of ∼15 M<SUB>☉</SUB>, kinetic energy of ∼1.4 foe, and an initial radius of ∼400 R<SUB>☉</SUB>. | en_US |
dc.language.iso | eng | en_US |
dc.title | SN 2016B a.k.a. ASASSN-16ab: a transitional Type II supernova | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stz949 | en_US |
dc.identifier.scopus | 2-s2.0-85067986201 | en_US |
dc.identifier.isi | 000474899400106 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/486/2/2850/5476505 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 486 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2850 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019MNRAS.486.2850D | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0002-3697-2616 | - |
crisitem.author.orcid | 0000-0002-3256-0016 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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File | Descrizione | Dimensioni | Formato | |
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1904.01844.pdf | preprint | 5.13 MB | Adobe PDF | Visualizza/apri |
stz949.pdf | pdf editoriale | 3.74 MB | Adobe PDF | Visualizza/apri |
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