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SN 2019muj-a well-o...
SN 2019muj-a well-observed Type Iax supernova that bridges the luminosity gap of the class
- Article/chapterEnglish2021
Publisher, publication year, extent ...
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2020-11-13
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Oxford University Press (OUP),2021
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printrdacarrier
Numbers
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LIBRIS-ID:oai:DiVA.org:su-191329
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https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-191329URI
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https://doi.org/10.1093/mnras/staa3543DOI
Supplementary language notes
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Language:English
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Summary in:English
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Subject category:ref swepub-contenttype
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Subject category:art swepub-publicationtype
Notes
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We present early-time (t < +50 d) observations of SN 2019muj (=ASASSN-19tr), one of the best-observed members of the peculiar SN Iax class. Ultraviolet and optical photometric and optical and near-infrared spectroscopic follow-up started from similar to 5 d before maximum light [t(max)(B) on 58707.8 MJD] and covers the photospheric phase. The early observations allow us to estimate the physical properties of the ejecta and characterize the possible divergence from a uniform chemical abundance structure. The estimated bolometric light-curve peaks at 1.05 x 10(42) erg s(-1) and indicates that only 0.031 M-circle dot of Ni-56 was produced, making SN 2019muj a moderate luminosity object in the Iax class with peak absolute magnitude of M-V = -16.4 mag. The estimated date of explosion is t(0) = 58698.2 MJD and implies a short rise time of t(rise) = 9.6 d in B band. We fit of the spectroscopic data by synthetic spectra, calculated via the radiative transfer code TARDIS. Adopting the partially stratified abundance template based on brighter SNe Iax provides a good match with SN 2019muj. However, without earlier spectra, the need for stratification cannot be stated in most of the elements, except carbon, which is allowed to appear in the outer layers only. SN 2019muj provides a unique opportunity to link extremely low-luminosity SNe Iax to well-studied, brighter SNe Iax.
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Szalai, Tamas
(author)
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Jha, Saurabh W.
(author)
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Camacho-Neves, Yssavo
(author)
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Kwok, Lindsey
(author)
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Foley, Ryan J.
(author)
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Kilpatrick, Charles D.
(author)
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Coulter, David A.
(author)
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Dimitriadis, Georgios
(author)
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Rest, Armin
(author)
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Rojas-Bravo, Cesar
(author)
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Siebert, Matthew R.
(author)
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Brown, Peter J.
(author)
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Burke, Jamison
(author)
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Gonzalez, Estefania Padilla
(author)
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Hiramatsu, Daichi
(author)
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Howell, D. Andrew
(author)
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McCully, Curtis
(author)
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Pellegrino, Craig
(author)
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Dobson, Matthew
(author)
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Smartt, Stephen J.
(author)
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Swift, Jonathan J.
(author)
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Stacey, Holland
(author)
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Rahman, Mohammed
(author)
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Sand, David J.
(author)
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Andrews, Jennifer
(author)
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Wyatt, Samuel
(author)
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Hsiao, Eric Y.
(author)
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Anderson, Joseph P.
(author)
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Chen, Ting-WanStockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)jach1916
(author)
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Della Valle, Massimo
(author)
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Galbany, Lluis
(author)
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Gromadzki, Mariusz
(author)
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Inserra, Cosimo
(author)
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Lyman, Joe
(author)
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Magee, Mark
(author)
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Maguire, Kate
(author)
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Mueller-Bravo, Tomas E.
(author)
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Nicholl, Matt
(author)
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Srivastav, Shubham
(author)
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Williams, Steven C.
(author)
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Stockholms universitetInstitutionen för astronomi
(creator_code:org_t)
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In:Monthly notices of the Royal Astronomical Society: Oxford University Press (OUP)501:1, s. 1078-10990035-87111365-2966
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Barna, Barnabas
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Szalai, Tamas
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Jha, Saurabh W.
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Camacho-Neves, Y ...
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Kwok, Lindsey
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Foley, Ryan J.
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Kilpatrick, Char ...
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Coulter, David A ...
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Dimitriadis, Geo ...
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Rest, Armin
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Rojas-Bravo, Ces ...
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Siebert, Matthew ...
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Brown, Peter J.
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Burke, Jamison
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Gonzalez, Estefa ...
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Hiramatsu, Daich ...
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Howell, D. Andre ...
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McCully, Curtis
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Pellegrino, Crai ...
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Dobson, Matthew
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Smartt, Stephen ...
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Swift, Jonathan ...
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Stacey, Holland
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Rahman, Mohammed
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Sand, David J.
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Andrews, Jennife ...
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Wyatt, Samuel
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Hsiao, Eric Y.
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Anderson, Joseph ...
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Chen, Ting-Wan
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Della Valle, Mas ...
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Galbany, Lluis
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Gromadzki, Mariu ...
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Inserra, Cosimo
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Lyman, Joe
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Magee, Mark
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Maguire, Kate
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Mueller-Bravo, T ...
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Nicholl, Matt
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Srivastav, Shubh ...
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- NATURAL SCIENCES
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NATURAL SCIENCES
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Stockholm University