Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt

Wang 王, Lingzhi 灵芝; Hu, Maokai; Wang, Lifan; Yang 杨, Yi 轶.; Yang, Jiawen; Gomez, Haley; Chen, Sijie; Hu, Lei; Chen, Ting-Wan; Mo, Jun; Wang, Xiaofeng; Baade, Dietrich; Hoeflich, Peter; Wheeler, J. Craig; Pignata, Giuliano; Burke, Jamison; Hiramatsu, Daichi; Howell, D. Andrew; McCully, Curtis; Pellegrino, Craig; Galbany, Lluís; Hsiao, Eric Y.; Sand, David J.; Zhang, Jujia; Uddin, Syed A.; Anderson, J. P.; Ashall, Chris; Cheng, Cheng; Gromadzki, Mariusz; Inserra, Cosimo; Lin, Han; Morrell, N.; Morales-Garoffolo, Antonia; Müller-Bravo, T. E.; Nicholl, Matt; Gonzalez, Estefania Padilla; Phillips, M. M.; Pineda-García, J.; Sai, Hanna; Smith, Mathew; Shahbandeh, M.; Srivastav, Shubham; Stritzinger, M. D.; Yang, Sheng; Young, D. R.; Yu, Lixin; Zhang, Xinghan

doi:10.1038/s41550-024-02197-9

Title: Newly formed dust within the circumstellar environment of SN Ia-CSM 2018evt

Journal Article · 09 February 2024 · Nature Astronomy

DOI: https://doi.org/10.1038/s41550-024-02197-9 · OSTI ID:2472337

^[1]; Hu, Maokai ^[2]; Wang, Lifan ^[3];

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^[5]; Chen, Sijie ^[3];

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^[7]; Mo, Jun ^[8];

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^[11]; Wheeler, J. Craig ^[12]; Pignata, Giuliano ^[13]; Burke, Jamison ^[14];

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Chinese Academy of Sciences South America Center for Astronomy (CASSACA), Beijing (China); OSTI
Chinese Academy of Sciences, Nanjing, Jiangsu (China). Purple Mountain Observatory
Texas A & M Univ., College Station, TX (United States)
Tsinghua Univ., Beijing (China); University of California, Berkeley, CA (United States)
Cardiff Univ., Wales (United Kingdom)
Chinese Academy of Sciences, Nanjing, Jiangsu (China). Purple Mountain Observatory; Carnegie Mellon Univ., Pittsburgh, PA (United States)
National Central Univ., Jhongli (Taiwan)
Tsinghua Univ., Beijing (China)
Tsinghua Univ., Beijing (China); Beijing Academy of Science and Technology (China)
European Organization for Astronomical Research in the Southern Hemisphere (ESO), Munich (Germany)
Florida State Univ., Tallahassee, FL (United States)
Univ. of Texas, Austin, TX (United States)
University Tarapaca, Arica (Chile); Millennium Institute of Astrophysics (MAS), Santiago (Chile)
Las Cumbres Observatory, Goleta, CA (United States); Univ. of California, Santa Barbara, CA (United States)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Las Cumbres Observatory, Goleta, CA (United States)
Institute of Space Sciences, Barcelona (Spain); Institut d'Estudis Espacials de Catalunya (IEEC), Barcelona (Spain)
Chinese Academy of Sciences (CAS), Kunming (China). Yunnan Observatories
Univ. of Arizona, Tucson, AZ (United States)
University Tarapaca, Arica (Chile); European Southern Observatory, Santiago (Chile)
Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States)
Chinese Academy of Sciences South America Center for Astronomy (CASSACA), Beijing (China)
Univ. of Warsaw (Poland)
Las Campanas Observatory, La Serena (Chile)
University of Cadiz (Spain)
Queen's Univ., Belfast, Northern Ireland (United Kingdom)
Millennium Institute of Astrophysics (MAS), Santiago (Chile); Univ. Andres Bello, Santiago (Chile)
University of Lyon, Villeurbanne (France)
Space Telescope Science Institute, Baltimore, MD (United States)
Aarhus Univ. (Denmark)
Henan Academy of Sciences, Zhengzhou (China)

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. Our model suggests enhanced CSM dust concentration at increasing distances from the SN as compared to what can be expected from the density profile of the mass loss from a steady stellar wind. By the time of the last mid-infrared observations at day +1,041, a total amount of 1.2 ± 0.2 × 10^-2 M_⊙ of new dust has been formed by SN 2018evt, making SN 2018evt one of the most prolific dust factories among supernovae with evidence of dust formation. The unprecedented witness of the intense production procedure of dust may shed light on the perceptions of dust formation in cosmic history.

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Research Organization:: Univ. of Texas, Austin, TX (United States)

Sponsoring Organization:: USDOE National Nuclear Security Administration (NNSA); National Science Foundation (NSF); National Natural Science Foundation of China; Chinese Academy of Sciences

Grant/Contract Number:: NA0003843

OSTI ID:: 2472337

Journal Information:: Nature Astronomy, Journal Name: Nature Astronomy Journal Issue: 4 Vol. 8; ISSN 2397-3366

Publisher:: Springer NatureCopyright Statement

Country of Publication:: United States

Language:: English

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A Long-duration Luminous Type IIn Supernova KISS15s: Strong Recombination Lines from the Inhomogeneous Ejecta–CSM Interaction Region and Hot Dust Emission from Newly Formed Dust Kokubo, Mitsuru; Mitsuda, Kazuma; Morokuma, Tomoki The Astrophysical Journal, Vol. 872, Issue 2 https://doi.org/10.3847/1538-4357/aaff6b	journal	February 2019
The Cold and Dusty Circumstellar Matter around Fast-expanding Type Ia Supernovae Wang, Xiaofeng; Chen, Jia; Wang, Lifan The Astrophysical Journal, Vol. 882, Issue 2 https://doi.org/10.3847/1538-4357/ab26b5	journal	September 2019
Optical and Near-infrared Observations of the Nearby SN Ia 2017cbv Wang, Lingzhi; Contreras, Carlos; Hu, Maokai The Astrophysical Journal, Vol. 904, Issue 1 https://doi.org/10.3847/1538-4357/abba82	journal	November 2020
The Infrared Echo of SN2010jl and Its Implications for Shock Breakout Characteristics Dwek, Eli; Sarangi, Arkaprabha; Arendt, Richard G. The Astrophysical Journal, Vol. 917, Issue 2 https://doi.org/10.3847/1538-4357/ac09ea	journal	August 2021
Spitzer’s Last Look at Extragalactic Explosions: Long-term Evolution of Interacting Supernovae Szalai, Tamás; Fox, Ori D.; Arendt, Richard G. The Astrophysical Journal, Vol. 919, Issue 1 https://doi.org/10.3847/1538-4357/ac0e2b	journal	September 2021
Less Than 1% of Core-collapse Supernovae in the Local Universe Occur in Elliptical Galaxies Irani, I.; Prentice, S. J.; Schulze, S. The Astrophysical Journal, Vol. 927, Issue 1 https://doi.org/10.3847/1538-4357/ac4709	journal	March 2022
Dust Production in a Thin Dense Shell in Supernovae with Early Circumstellar Interactions Sarangi, Arkaprabha; Slavin, Jonathan D. The Astrophysical Journal, Vol. 933, Issue 1 https://doi.org/10.3847/1538-4357/ac713d	journal	July 2022
Image Subtraction in Fourier Space Hu, Lei; Wang, Lifan; Chen, Xingzhuo The Astrophysical Journal, Vol. 936, Issue 2 https://doi.org/10.3847/1538-4357/ac7394	journal	September 2022
The Absolute Magnitudes of 1991T-like Supernovae ^* Phillips, M. M.; Ashall, C.; Burns, Christopher R. The Astrophysical Journal, Vol. 938, Issue 1 https://doi.org/10.3847/1538-4357/ac9305	journal	October 2022
A Systematic Study of Ia-CSM Supernovae from the ZTF Bright Transient Survey Sharma, Yashvi; Sollerman, Jesper; Fremling, Christoffer The Astrophysical Journal, Vol. 948, Issue 1 https://doi.org/10.3847/1538-4357/acbc16	journal	May 2023
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ICORE: Image Co-addition with Optional Resolution Enhancement Masci, Frank arXiv https://doi.org/10.48550/arXiv.1301.2718	preprint	January 2013
Newly Formed Dust within the Circumstellar Environment of SNIa-CSM 2018evt Wang, Lingzhi; Hu, Maokai; Wang, Lifan Science Data Bank https://doi.org/10.57760/sciencedb.07968	dataset	January 2024
Newly Formed Dust within the Cosmic Dust Storms of SNIa-CSM 2018evt Wang, Lingzhi; Hu, Maokai; Wang, Lifan figshare https://doi.org/10.6084/m9.figshare.21543558	dataset	January 2024

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