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Sökning: WFRF:(Pellegrino Craig) > SN 2019muj-a well-o...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004403naa a2200805 4500
001oai:DiVA.org:su-191329
003SwePub
008210316s2021 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1913292 URI
024a https://doi.org/10.1093/mnras/staa35432 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Barna, Barnabas4 aut
2451 0a SN 2019muj-a well-observed Type Iax supernova that bridges the luminosity gap of the class
264 c 2020-11-13
264 1b Oxford University Press (OUP),c 2021
338 a print2 rdacarrier
520 a 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.
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a supernovae: general
653 a supernovae: individual: SN 2019muj (ASASSN-19tr)
700a Szalai, Tamas4 aut
700a Jha, Saurabh W.4 aut
700a Camacho-Neves, Yssavo4 aut
700a Kwok, Lindsey4 aut
700a Foley, Ryan J.4 aut
700a Kilpatrick, Charles D.4 aut
700a Coulter, David A.4 aut
700a Dimitriadis, Georgios4 aut
700a Rest, Armin4 aut
700a Rojas-Bravo, Cesar4 aut
700a Siebert, Matthew R.4 aut
700a Brown, Peter J.4 aut
700a Burke, Jamison4 aut
700a Gonzalez, Estefania Padilla4 aut
700a Hiramatsu, Daichi4 aut
700a Howell, D. Andrew4 aut
700a McCully, Curtis4 aut
700a Pellegrino, Craig4 aut
700a Dobson, Matthew4 aut
700a Smartt, Stephen J.4 aut
700a Swift, Jonathan J.4 aut
700a Stacey, Holland4 aut
700a Rahman, Mohammed4 aut
700a Sand, David J.4 aut
700a Andrews, Jennifer4 aut
700a Wyatt, Samuel4 aut
700a Hsiao, Eric Y.4 aut
700a Anderson, Joseph P.4 aut
700a Chen, Ting-Wanu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)jach1916
700a Della Valle, Massimo4 aut
700a Galbany, Lluis4 aut
700a Gromadzki, Mariusz4 aut
700a Inserra, Cosimo4 aut
700a Lyman, Joe4 aut
700a Magee, Mark4 aut
700a Maguire, Kate4 aut
700a Mueller-Bravo, Tomas E.4 aut
700a Nicholl, Matt4 aut
700a Srivastav, Shubham4 aut
700a Williams, Steven C.4 aut
710a Stockholms universitetb Institutionen för astronomi4 org
773t Monthly notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 501:1, s. 1078-1099q 501:1<1078-1099x 0035-8711x 1365-2966
856u http://real.mtak.hu/131343/1/2011.03068.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-191329
8564 8u https://doi.org/10.1093/mnras/staa3543

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