Lingzhi 灵芝 Wang王, Maokai Hu, Lifan Wang, Yi 轶 Yang 杨, Jiawen Yang, Haley Gomez, Sijie Chen, Lei Hu, Ting-Wan Chen, Jun Mo, Xiaofeng Wang, Dietrich Baade, Peter Hoeflich, J Craig Wheeler, Giuliano Pignata, Jamison Burke, Daichi Hiramatsu, D Andrew Howell, Curtis McCully, Craig Pellegrino, Lluís Galbany, Eric Y Hsiao, David J Sand, Jujia Zhang, Syed A Uddin, J P Anderson, Chris Ashall, Cheng Cheng, Mariusz Gromadzki, Cosimo Inserra, Han Lin, N Morrell, Antonia Morales-Garoffolo, T E Müller-Bravo, Matt Nicholl, Estefania Padilla Gonzalez, M M Phillips, J Pineda-García, Hanna Sai, Mathew Smith, M Shahbandeh, Shubham Srivastav, M D Stritzinger, Sheng Yang, D R Young, Lixin Yu, Xinghan Zhang
Dust associated with various stellar sources in galaxies at all cosmic epochs remains a controversial topic, particularly whether supernovae play an important role in dust production. We report evidence of dust formation in the cold, dense shell behind the ejecta-circumstellar medium (CSM) interaction in the Type Ia-CSM supernova (SN) 2018evt three years after the explosion, characterized by a rise in mid-infrared emission accompanied by an accelerated decline in the optical radiation of the SN. Such a dust-formation picture is also corroborated by the concurrent evolution of the profiles of the Hα emission line...
2024: Nature Astronomy