Serendipitous detection of the dusty Type IIL SN 1980K with <i>JWST</i>/MIRI-Reference-Cited by-同舟云学术

Serendipitous detection of the dusty Type IIL SN 1980K with JWST/MIRI

Published:2024-02-21 Issue:1 Volume:529 Page:155-168
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Zsíros Szanna¹^ORCID,Szalai Tamás¹²^ORCID,De Looze Ilse³^ORCID,Sarangi Arkaprabha⁴^ORCID,Shahbandeh Melissa⁵⁶^ORCID,Fox Ori D⁶^ORCID,Temim Tea⁷^ORCID,Milisavljevic Dan⁸⁹^ORCID,Van Dyk Schuyler D¹⁰^ORCID,Smith Nathan¹¹^ORCID,Filippenko Alexei V¹²^ORCID,Brink Thomas G¹²^ORCID,Zheng WeiKang¹²,Dessart Luc¹³,Jencson Jacob⁵^ORCID,Johansson Joel¹⁴^ORCID,Pierel Justin⁶,Rest Armin⁵⁶^ORCID,Tinyanont Samaporn¹⁵¹⁶^ORCID,Niculescu-Duvaz Maria¹⁷,Barlow M J¹⁷^ORCID,Wesson Roger¹⁸^ORCID,Andrews Jennifer¹⁹,Clayton Geoff²⁰^ORCID,De Kishalay²¹,Dwek Eli²²,Engesser Michael⁶,Foley Ryan J¹⁵,Gezari Suvi⁶,Gomez Sebastian⁶^ORCID,Gonzaga Shireen⁶,Kasliwal Mansi²³^ORCID,Lau Ryan²⁴,Marston Anthony²⁵,O’Steen Richard⁶,Siebert Matthew⁶,Skrutskie Michael²⁶,Strolger Lou⁶,Wang Qinan⁵^ORCID,Williams Brian²²,Williams Robert⁶,Xiao Lin²⁷²⁸^ORCID

Affiliation:

1. Department of Experimental Physics, Institute of Physics, University of Szeged , H-6720 Szeged, Dóm tér 9 , Hungary

2. HUN-REN–SZTE Stellar Astrophysics Research Group , H-6500 Baja, Szegedi út, Kt. 766 , Hungary

3. Sterrenkundig Observatorium, Ghent University , Krijgslaan 281 – S9, B-9000 Gent , Belgium

4. DARK, Niels Bohr Institute, University of Copenhagen , Jagtvej 128, DK-2200 Copenhagen , Denmark

5. Department of Physics and Astronomy, Johns Hopkins University , Baltimore, MD 21218 , USA

6. Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218 , USA

7. Department of Astrophysical Sciences, Princeton University , Princeton, NJ 08544 , USA

8. Purdue University, Department of Physics and Astronomy , 525 Northwestern Ave, West Lafayette, IN 47907 , USA

9. Integrative Data Science Initiative, Purdue University , West Lafayette, IN 47907 , USA

10. Caltech/IPAC , Mailcode 100-22, Pasadena, CA 91125 , USA

11. Steward Observatory, University of Arizona , 933 N. Cherry St, Tucson, AZ 85721 , USA

12. Department of Astronomy, University of California , Berkeley, CA 94720-3411 , USA

13. Institut d’Astrophysique de Paris , CNRS–Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris , France

14. Oskar Klein Centre, Department of Physics, Stockholm University , AlbaNova, SE-10691 Stockholm , Sweden

15. Department of Astronomy and Astrophysics, University of California , Santa Cruz, CA 95064 , USA

16. National Astronomical Research Institute of Thailand , 260 Moo 4, Donkaew, Maerim, Chiang Mai, 50180 , Thailand

17. Department of Physics & Astronomy, University College London , Gower St, London WC1E 6BT , UK

18. School of Physics and Astronomy, Cardiff University , Queen’s Buildings, The Parade, Cardiff, CF24 3AA , UK

19. Gemini Observatory , 670 N. Aohoku Place, Hilo, Hawaii, 96720 , USA

20. Physics & Astronomy, Louisiana State University , Baton Rouge, LA , USA

21. MIT-Kavli Institute for Astrophysics and Space Research , 77 Massachusetts Ave., Cambridge, MA 02139 , USA

22. Observational Cosmology Lab, NASA Goddard Space Flight Center , Code 665, Greenbelt, MD 20771 , USA

23. Cahill Center for Astrophysics, California Institute of Technology , 1200 E. California Blvd. Pasadena, CA 91125 , USA

24. NSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, 85719, AZ , USA

25. European Space Agency (ESA) , ESAC, E-28692 Villanueva de la Canada, Madrid , Spain

26. Department of Astronomy, University of Virginia , Charlottesville, VA 22904-4325 , USA

27. Department of Physics, College of Physical Sciences and Technology, Hebei University , Wusidong Road 180, Baoding 071002 , China

28. Key Laboratory of High-precision Computation and Application of Quantum Field Theory of Hebei Province, Hebei University , Baoding 071002 , China

Abstract

ABSTRACT We present mid-infrared (mid-IR) imaging of the Type IIL supernova (SN) 1980K with the JWST more than 40 yr post-explosion. SN 1980K, located in the nearby (D ≈ 7 Mpc) ‘SN factory’ galaxy NGC 6946, was serendipitously captured in JWST/MIRI images taken of the field of SN 2004et in the same galaxy. SN 1980K serves as a promising candidate for studying the transitional phase between young SNe and older SN remnants and also provides a great opportunity to investigate its the close environment. SN 1980K can be identified as a clear and bright point source in all eight MIRI filters from F560W up to F2550W. We fit analytical dust models to the mid-IR spectral energy distribution that reveal a large amount (Md ≈ 0.002 M⊙) of Si-dominated dust at $T_\rm {dust}\approx 150$ K (accompanied by a hotter dust/gas component), and also computed numerical SED dust models. Radiative transfer modelling of a late-time optical spectrum obtained recently with Keck discloses that an even larger (∼0.24–0.58 M⊙) amount of dust is needed in order for selective extinction to explain the asymmetric line profile shapes observed in SN 1980K. As a conclusion, with JWST, we may see i) pre-existing circumstellar dust heated collisionally (or, partly radiatively), analogous to the equatorial ring of SN 1987A, or ii) the mid-IR component of the presumed newly-formed dust, accompanied by much more colder dust present in the ejecta (as suggested by the late-time the optical spectra).

Funder

NASA

ESA

CSA

Space Telescope Science Institute

Publisher

Oxford University Press (OUP)

Link

https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stae507/56732877/stae507.pdf

Reference102 articles.

1. CHARACTERIZING THEV-BAND LIGHT-CURVES OF HYDROGEN-RICH TYPE II SUPERNOVAE

2. EVIDENCE FOR PRE-EXISTING DUST IN THE BRIGHT TYPE IIn SN 2010jl

3. Inferring properties of dust in supernovae with neural networks

4. INTERSTELLAR AND EJECTA DUST IN THE CAS A SUPERNOVA REMNANT

5. INFRARED CONTINUUM AND LINE EVOLUTION OF THE EQUATORIAL RING AROUND SN 1987A