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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 06072naa a2201441 4500 | |
| 001 | oai:DiVA.org:su-185472 | |
| 003 | SwePub | |
| 008 | 201021s2020 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1854722 URI |
| 024 | 7 | a https://doi.org/10.1093/mnras/staa14522 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Gutierrez, C. P.4 aut |
| 245 | 1 0 | a DES16C3cje :b A low-luminosity, long-lived supernova |
| 264 | c 2020-05-25 | |
| 264 | 1 | b Oxford University Press (OUP),c 2020 |
| 338 | a print2 rdacarrier | |
| 520 | a We present DES16C3cje, a low-luminosity, long-lived type II supernova (SN II) at redshift 0.0618, detected by the Dark Energy Survey (DES). DES16C3cje is a unique SN. The spectra are characterized by extremely narrow photospheric lines corresponding to very low expansion velocities of less than or similar to 1500 km s(-1), and the light curve shows an initial peak that fades after 50 d before slowly rebrightening over a further 100 d to reach an absolute brightness of M-r similar to 15.5 mag. The decline rate of the late-time light curve is then slower than that expected from the powering by radioactive decay of Co-56, but is comparable to that expected from accretion power. Comparing the bolometric light curve with hydrodynamical models, we find that DES16C3cje can be explained by either (i) a low explosion energy (0.11 foe) and relatively large Ni-56 production of 0.075 M-circle dot from an similar to 15 M-circle dot red supergiant progenitor typical of other SNe II, or (ii) a relatively compact similar to 40 M-circle dot star, explosion energy of 1 foe, and 0.08 M-circle dot of Ni-56. Both scenarios require additional energy input to explain the late-time light curve, which is consistent with fallback accretion at a rate of similar to 0.5 x 10(-)(8) M-circle dot s(-1). | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a supernovae: general | |
| 653 | a supernovae: individual: (DES16C3cje) | |
| 700 | 1 | a Sullivan, M.4 aut |
| 700 | 1 | a Martinez, L.4 aut |
| 700 | 1 | a Bersten, M. C.4 aut |
| 700 | 1 | a Inserra, C.4 aut |
| 700 | 1 | a Smith, M.4 aut |
| 700 | 1 | a Anderson, J. P.4 aut |
| 700 | 1 | a Pan, Y.-C.4 aut |
| 700 | 1 | a Pastorello, A.4 aut |
| 700 | 1 | a Galbany, L.4 aut |
| 700 | 1 | a Nugent, P.4 aut |
| 700 | 1 | a Angus, C. R.4 aut |
| 700 | 1 | a Barbarino, Cristinau Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)cbarb |
| 700 | 1 | a Carollo, D.4 aut |
| 700 | 1 | a Chen, T.-W.4 aut |
| 700 | 1 | a Davis, T. M.4 aut |
| 700 | 1 | a Della Valle, M.4 aut |
| 700 | 1 | a Foley, R. J.4 aut |
| 700 | 1 | a Fraser, M.4 aut |
| 700 | 1 | a Frohmaier, C.4 aut |
| 700 | 1 | a Gonzalez-Gaitan, S.4 aut |
| 700 | 1 | a Gromadzki, M.4 aut |
| 700 | 1 | a Kankare, E.4 aut |
| 700 | 1 | a Kokotanekova, R.4 aut |
| 700 | 1 | a Kollmeier, J.4 aut |
| 700 | 1 | a Lewis, G. F.4 aut |
| 700 | 1 | a Magee, M. R.4 aut |
| 700 | 1 | a Maguire, K.4 aut |
| 700 | 1 | a Moller, A.4 aut |
| 700 | 1 | a Morrell, N.4 aut |
| 700 | 1 | a Nicholl, M.4 aut |
| 700 | 1 | a Pursiainen, M.4 aut |
| 700 | 1 | a Sollerman, Jesperu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)solle |
| 700 | 1 | a Sommer, N. E.4 aut |
| 700 | 1 | a Swann, E.4 aut |
| 700 | 1 | a Tucker, B. E.4 aut |
| 700 | 1 | a Wiseman, P.4 aut |
| 700 | 1 | a Aguena, M.4 aut |
| 700 | 1 | a Allam, S.4 aut |
| 700 | 1 | a Avila, S.4 aut |
| 700 | 1 | a Bertin, E.4 aut |
| 700 | 1 | a Brooks, D.4 aut |
| 700 | 1 | a Buckley-Geer, E.4 aut |
| 700 | 1 | a Burke, D. L.4 aut |
| 700 | 1 | a Rosell, A. Carnero4 aut |
| 700 | 1 | a Kind, M. Carrasco4 aut |
| 700 | 1 | a Carretero, J.4 aut |
| 700 | 1 | a Costanzi, M.4 aut |
| 700 | 1 | a da Costa, L. N.4 aut |
| 700 | 1 | a De Vicente, J.4 aut |
| 700 | 1 | a Desai, S.4 aut |
| 700 | 1 | a Diehl, H. T.4 aut |
| 700 | 1 | a Doel, P.4 aut |
| 700 | 1 | a Eifler, T. F.4 aut |
| 700 | 1 | a Flaugher, B.4 aut |
| 700 | 1 | a Fosalba, P.4 aut |
| 700 | 1 | a Frieman, J.4 aut |
| 700 | 1 | a Garcia-Bellido, J.4 aut |
| 700 | 1 | a Gerdes, D. W.4 aut |
| 700 | 1 | a Gruen, D.4 aut |
| 700 | 1 | a Gruendl, R. A.4 aut |
| 700 | 1 | a Gschwend, J.4 aut |
| 700 | 1 | a Gutierrez, G.4 aut |
| 700 | 1 | a Hinton, S. R.4 aut |
| 700 | 1 | a Hollowood, D. L.4 aut |
| 700 | 1 | a Honscheid, K.4 aut |
| 700 | 1 | a James, D. J.4 aut |
| 700 | 1 | a Kuehn, K.4 aut |
| 700 | 1 | a Kuropatkin, N.4 aut |
| 700 | 1 | a Lahav, O.4 aut |
| 700 | 1 | a Lima, M.4 aut |
| 700 | 1 | a Maia, M. A. G.4 aut |
| 700 | 1 | a March, M.4 aut |
| 700 | 1 | a Menanteau, F.4 aut |
| 700 | 1 | a Miquel, R.4 aut |
| 700 | 1 | a Morganson, E.4 aut |
| 700 | 1 | a Palmese, A.4 aut |
| 700 | 1 | a Paz-Chinchon, F.4 aut |
| 700 | 1 | a Plazas, A. A.4 aut |
| 700 | 1 | a Sako, M.4 aut |
| 700 | 1 | a Sanchez, E.4 aut |
| 700 | 1 | a Scarpine, V.4 aut |
| 700 | 1 | a Schubnell, M.4 aut |
| 700 | 1 | a Serrano, S.4 aut |
| 700 | 1 | a Sevilla-Noarbe, I.4 aut |
| 700 | 1 | a Soares-Santos, M.4 aut |
| 700 | 1 | a Suchyta, E.4 aut |
| 700 | 1 | a Swanson, M. E. C.4 aut |
| 700 | 1 | a Tarle, G.4 aut |
| 700 | 1 | a Thomas, D.4 aut |
| 700 | 1 | a Varga, T. N.4 aut |
| 700 | 1 | a Walker, A. R.4 aut |
| 700 | 1 | a Wilkinson, R.4 aut |
| 710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
| 773 | 0 | t Monthly notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 496:1, s. 95-110q 496:1<95-110x 0035-8711x 1365-2966 |
| 856 | 4 | u https://doi.org/10.1093/mnras/staa1452y Fulltext |
| 856 | 4 | u https://orca.cardiff.ac.uk/132495/1/staa1452.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-185472 |
| 856 | 4 8 | u https://doi.org/10.1093/mnras/staa1452 |
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