Sökning: WFRF:(Angulo A) > Revealing the Proge...
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000 | 04075naa a2200817 4500 | |
001 | oai:DiVA.org:su-215889 | |
003 | SwePub | |
008 | 230330s2023 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2158892 URI |
024 | 7 | a https://doi.org/10.3847/2041-8213/acb0d02 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 Wang, Qinan4 aut |
245 | 1 0 | a Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve |
264 | c 2023-01-31 | |
264 | 1 | b American Astronomical Society,c 2023 |
338 | a print2 rdacarrier | |
520 | a We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence. We present optical and near-infrared spectral series of SN 2021zby, including three spectra during the shock-cooling phase. Using a multiband model fit, we find that the inferred properties of its progenitor are consistent with a red supergiant or yellow supergiant, with an envelope mass of ∼0.30–0.65 M⊙ and an envelope radius of ∼120–300 R⊙. These inferred progenitor properties are similar to those of other SNe IIb with a double-peaked feature, such as SNe 1993J, 2011dh, 2016gkg, and 2017jgh. This study further validates the importance of the high cadence and early coverage in resolving the shape of the shock-cooling light curve, while the multiband observations, particularly UV, are also necessary to fully constrain the progenitor properties. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
700 | 1 | a Armstrong, Patrick4 aut |
700 | 1 | a Zenati, Yossef4 aut |
700 | 1 | a Ridden-Harper, Ryan4 aut |
700 | 1 | a Rest, Armin4 aut |
700 | 1 | a Arcavi, Iair4 aut |
700 | 1 | a Kilpatrick, Charles D.4 aut |
700 | 1 | a Foley, Ryan J.4 aut |
700 | 1 | a Tucker, Brad E.4 aut |
700 | 1 | a Lidman, Chris4 aut |
700 | 1 | a Killestein, Thomas L.4 aut |
700 | 1 | a Shahbandeh, Melissa4 aut |
700 | 1 | a Anderson, Joseph P.4 aut |
700 | 1 | a Angulo, Rodrigo4 aut |
700 | 1 | a Ashall, Chris4 aut |
700 | 1 | a Burke, Jamison4 aut |
700 | 1 | a Chen, Ting-Wanu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)jach1916 |
700 | 1 | a von Coelln, Sophie4 aut |
700 | 1 | a Dalrymple, Kyle A.4 aut |
700 | 1 | a Davis, Kyle W.4 aut |
700 | 1 | a Fulton, Michael D.4 aut |
700 | 1 | a Galbany, Lluís4 aut |
700 | 1 | a Gonzalez, Estefania Padilla4 aut |
700 | 1 | a Gao, Bore4 aut |
700 | 1 | a Gromadzki, Mariusz4 aut |
700 | 1 | a Howell, D. Andrew4 aut |
700 | 1 | a Ihanec, Nada4 aut |
700 | 1 | a Jencson, Jacob E.4 aut |
700 | 1 | a Jones, David O.4 aut |
700 | 1 | a Lyman, Joseph D.4 aut |
700 | 1 | a McCully, Curtis4 aut |
700 | 1 | a Müller-Bravo, Tomás E.4 aut |
700 | 1 | a Newsome, Megan4 aut |
700 | 1 | a Nicholl, Matt4 aut |
700 | 1 | a O'Neill, David4 aut |
700 | 1 | a Pellegrino, Craig4 aut |
700 | 1 | a Rest, Sofia4 aut |
700 | 1 | a Smartt, Stephen J.4 aut |
700 | 1 | a Smith, Ken4 aut |
700 | 1 | a Srivastav, Shubham4 aut |
700 | 1 | a Terreran, Giacomo4 aut |
700 | 1 | a Tinyanont, Samaporn4 aut |
700 | 1 | a Young, David R.4 aut |
700 | 1 | a Zenteno, Alfredo4 aut |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Astrophysical Journal Lettersd : American Astronomical Societyg 943:2q 943:2x 2041-8205x 2041-8213 |
856 | 4 | u https://doi.org/10.3847/2041-8213/acb0d0y Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-215889 |
856 | 4 8 | u https://doi.org/10.3847/2041-8213/acb0d0 |
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