JWST MIRI Imager Observations of Supernova SN 1987A

There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 yr, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta, and the surrounding medium and to witness the birth of an SN remnant...

Full description

Bibliographic Details
Main Authors: P. Bouchet, R. Gastaud, A. Coulais, M. J. Barlow, C. Fransson, P. J. Kavanagh, J. Larsson, T. Temim, O. C. Jones, A. S. Hirschauer, T. Tikkanen, J. A. D. L. Blommaert, O. D. Fox, A. Glasse, N. Habel, J. Hjorth, J. Jaspers, O. Krause, R. M. Lau, L. Lenkić, M. Meixner, O. Nayak, A. Rest, B. Sargent, R. Wesson, G. S. Wright, L. Colina, E. F. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, G. Östlin, T. P. Ray, B. Vandenbussche
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad2770
_version_ 1797222372120461312
author P. Bouchet
R. Gastaud
A. Coulais
M. J. Barlow
C. Fransson
P. J. Kavanagh
J. Larsson
T. Temim
O. C. Jones
A. S. Hirschauer
T. Tikkanen
J. A. D. L. Blommaert
O. D. Fox
A. Glasse
N. Habel
J. Hjorth
J. Jaspers
O. Krause
R. M. Lau
L. Lenkić
M. Meixner
O. Nayak
A. Rest
B. Sargent
R. Wesson
G. S. Wright
L. Colina
E. F. van Dishoeck
M. Güdel
Th. Henning
P.-O. Lagage
G. Östlin
T. P. Ray
B. Vandenbussche
author_facet P. Bouchet
R. Gastaud
A. Coulais
M. J. Barlow
C. Fransson
P. J. Kavanagh
J. Larsson
T. Temim
O. C. Jones
A. S. Hirschauer
T. Tikkanen
J. A. D. L. Blommaert
O. D. Fox
A. Glasse
N. Habel
J. Hjorth
J. Jaspers
O. Krause
R. M. Lau
L. Lenkić
M. Meixner
O. Nayak
A. Rest
B. Sargent
R. Wesson
G. S. Wright
L. Colina
E. F. van Dishoeck
M. Güdel
Th. Henning
P.-O. Lagage
G. Östlin
T. P. Ray
B. Vandenbussche
author_sort P. Bouchet
collection DOAJ
description There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 yr, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta, and the surrounding medium and to witness the birth of an SN remnant (SNR). The James Webb Space Telescope, with its high spatial resolution and extreme sensitivity, gives a new view on these issues. We report on the first imaging observations obtained with the Mid-InfraRed Instrument (MIRI). We build temperature maps and discuss the morphology of the nascent SNR. Our results show that the temperatures in the equatorial ring (ER) are quite nonuniform. This could be due to dust destruction in some parts of the ring, as had been assumed in some previous works. We show that the IR emission extends beyond the ER, illustrating the fact that the shock wave has now passed through this ring to affect the circumstellar medium on a larger scale. Finally, while submillimeter Atacama Large Millimeter Array observations have hinted at the location of the compact remnant of SN 1987A, we note that our MIRI data have found no such evidence.
first_indexed 2024-04-24T13:20:17Z
format Article
id doaj.art-523ede7d35f64fc8a49e9fd61097e41d
institution Directory Open Access Journal
issn 1538-4357
language English
last_indexed 2024-04-24T13:20:17Z
publishDate 2024-01-01
publisher IOP Publishing
record_format Article
series The Astrophysical Journal
spelling doaj.art-523ede7d35f64fc8a49e9fd61097e41d2024-04-04T15:33:14ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-0196515110.3847/1538-4357/ad2770JWST MIRI Imager Observations of Supernova SN 1987AP. Bouchet0https://orcid.org/0000-0002-6018-3393R. Gastaud1https://orcid.org/0009-0007-5200-1362A. Coulais2https://orcid.org/0000-0001-6492-7719M. J. Barlow3https://orcid.org/0000-0002-3875-1171C. Fransson4https://orcid.org/0000-0001-8532-3594P. J. Kavanagh5https://orcid.org/0000-0001-6872-2358J. Larsson6https://orcid.org/0000-0003-0065-2933T. Temim7https://orcid.org/0000-0001-7380-3144O. C. Jones8https://orcid.org/0000-0003-4870-5547A. S. Hirschauer9https://orcid.org/0000-0002-2954-8622T. Tikkanen10https://orcid.org/0009-0003-6128-2347J. A. D. L. Blommaert11https://orcid.org/0000-0002-5797-2439O. D. Fox12https://orcid.org/0000-0003-2238-1572A. Glasse13https://orcid.org/0000-0002-2041-2462N. Habel14https://orcid.org/0000-0002-2667-1676J. Hjorth15https://orcid.org/0000-0002-4571-2306J. Jaspers16https://orcid.org/0000-0002-0577-1950O. Krause17R. M. Lau18https://orcid.org/0000-0003-0778-0321L. Lenkić19https://orcid.org/0000-0003-4023-8657M. Meixner20https://orcid.org/0000-0002-0522-3743O. Nayak21https://orcid.org/0000-0001-6576-6339A. Rest22https://orcid.org/0000-0002-4410-5387B. Sargent23https://orcid.org/0000-0001-9855-8261R. Wesson24https://orcid.org/0000-0002-4000-4394G. S. Wright25https://orcid.org/0000-0001-7416-7936L. Colina26https://orcid.org/0000-0002-9090-4227E. F. van Dishoeck27https://orcid.org/0000-0001-7591-1907M. Güdel28https://orcid.org/0000-0001-9818-0588Th. Henning29https://orcid.org/0000-0002-1493-300XP.-O. Lagage30G. Östlin31https://orcid.org/0000-0002-3005-1349T. P. Ray32https://orcid.org/0000-0002-2110-1068B. Vandenbussche33https://orcid.org/0000-0002-1368-3109Université Paris-Saclay, Université Paris Cité , CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, France ; Patrice.Bouchet@cea.frUniversité Paris-Saclay , CEA, DEDIP, 91191, Gif-sur-Yvette, FranceUniversité Paris-Saclay, Université Paris Cité , CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, France ; Patrice.Bouchet@cea.fr; LERMA, Observatoire de Paris, Université PSL , Sorbonne Université, CNRS, Paris, FranceDepartment of Physics and Astronomy, University College London (UCL) , Gower Street, London WC1E 6BT, UKDepartment of Astronomy, Stockholm University , The Oskar Klein Centre, AlbaNova, SE-106 91 Stockholm, SwedenDepartment of Experimental Physics, Maynooth University , Maynooth, Co. Kildare, Ireland; Dublin Institute for Advanced Studies , School of Cosmic Physics, Astronomy & Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, IrelandDepartment of Physics , KTH Royal Institute of Technology, The Oskar Klein Centre, AlbaNova, SE-106 91 Stockholm, SwedenDepartment of Astrophysical Sciences, Princeton University , Princeton, NJ 08544, USAUK Astronomy Technology Centre , Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UKSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USASchool of Physics & Astronomy, Space Research Centre, University of Leicester , Space Park Leicester, 92 Corporation Road, Leicester LE4 5SP, UKAstronomy and Astrophysics Research Group, Department of Physics and Astrophysics, Vrije Universiteit Brussel , Pleinlaan 2, B-1050 Brussels, BelgiumSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USAUK Astronomy Technology Centre , Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UKStratospheric Observatory for Infrared Astronomy , NASA Ames Research Center, Mail Stop 204-14, Moffett Field, CA 94035, USADARK, Niels Bohr Institute, University of Copenhagen , Jagtvej 128, 2200 Copenhagen, DenmarkDepartment of Experimental Physics, Maynooth University , Maynooth, Co. Kildare, Ireland; Dublin Institute for Advanced Studies , School of Cosmic Physics, Astronomy & Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, IrelandMax Planck Institute for Astronomy , Heidelberg (MPIA), GermanyNSF’s NOIR Lab 950 N. Cherry Avenue , Tucson, AZ 85721, USAStratospheric Observatory for Infrared Astronomy , NASA Ames Research Center, Mail Stop 204-14, Moffett Field, CA 94035, USAJet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Dr., Pasadena, CA 91109, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA; Department of Physics and Astronomy, Johns Hopkins University , 3400 North Charles Street, Baltimore, MD 21218, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA; Center for Astrophysical Sciences, The William H. Miller III Department of Physics and Astronomy, Johns Hopkins University , Baltimore, MD 21218, USASchool of Physics and Astronomy, Cardiff University , Queen’s Buildings, The Parade, Cardiff, CF24 3AA, UKUK Astronomy Technology Centre , Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UKCentro de Astrobiología (CAB) , CSIC-INTA, Ctra. de Ajalvir km 4, Torrejón de Ardoz, E-28850, Madrid, SpainMax-Planck Institut für Extraterresstrische Physic (MPE) , Giessenbachstr., 1, D-85748, Garching, Germany; Leiden Observatory, Leiden University , 2300 RA Leiden, The NetherlandsDept. of Astrophysics, University of Vienna , Türkenschanzstr. 17, A-1180 Vienna, Austria; Max-Planck-Institut für Astronomie (MPIA) , Königstuhl, 17, D-69117 Heidelberg, Germany; ETH Zürich , Institute for Particle Physics and Astrophysics, Wolfgang-Pauli Str., 27, 8093 Zürich, SwitzerlandMax-Planck Institut für Extraterresstrische Physic (MPE) , Giessenbachstr., 1, D-85748, Garching, GermanyUniversité Paris-Saclay, Université Paris Cité , CEA, CNRS, AIM, F-91191 Gif-sur-Yvette, France ; Patrice.Bouchet@cea.frDepartment of Astronomy, Stockholm University , The Oskar Klein Centre, AlbaNova, SE-106 91 Stockholm, SwedenDublin Institute for Advanced Studies , School of Cosmic Physics, Astronomy & Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, IrelandInstitute of Astronomy , KU Leuwen, Celestijnenlaan 200D, 3001 Leuwen, BelgiumThere exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 yr, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta, and the surrounding medium and to witness the birth of an SN remnant (SNR). The James Webb Space Telescope, with its high spatial resolution and extreme sensitivity, gives a new view on these issues. We report on the first imaging observations obtained with the Mid-InfraRed Instrument (MIRI). We build temperature maps and discuss the morphology of the nascent SNR. Our results show that the temperatures in the equatorial ring (ER) are quite nonuniform. This could be due to dust destruction in some parts of the ring, as had been assumed in some previous works. We show that the IR emission extends beyond the ER, illustrating the fact that the shock wave has now passed through this ring to affect the circumstellar medium on a larger scale. Finally, while submillimeter Atacama Large Millimeter Array observations have hinted at the location of the compact remnant of SN 1987A, we note that our MIRI data have found no such evidence.https://doi.org/10.3847/1538-4357/ad2770Type II supernovaeCore-collapse supernovaeSupernova remnants
spellingShingle P. Bouchet
R. Gastaud
A. Coulais
M. J. Barlow
C. Fransson
P. J. Kavanagh
J. Larsson
T. Temim
O. C. Jones
A. S. Hirschauer
T. Tikkanen
J. A. D. L. Blommaert
O. D. Fox
A. Glasse
N. Habel
J. Hjorth
J. Jaspers
O. Krause
R. M. Lau
L. Lenkić
M. Meixner
O. Nayak
A. Rest
B. Sargent
R. Wesson
G. S. Wright
L. Colina
E. F. van Dishoeck
M. Güdel
Th. Henning
P.-O. Lagage
G. Östlin
T. P. Ray
B. Vandenbussche
JWST MIRI Imager Observations of Supernova SN 1987A
The Astrophysical Journal
Type II supernovae
Core-collapse supernovae
Supernova remnants
title JWST MIRI Imager Observations of Supernova SN 1987A
title_full JWST MIRI Imager Observations of Supernova SN 1987A
title_fullStr JWST MIRI Imager Observations of Supernova SN 1987A
title_full_unstemmed JWST MIRI Imager Observations of Supernova SN 1987A
title_short JWST MIRI Imager Observations of Supernova SN 1987A
title_sort jwst miri imager observations of supernova sn 1987a
topic Type II supernovae
Core-collapse supernovae
Supernova remnants
url https://doi.org/10.3847/1538-4357/ad2770
work_keys_str_mv AT pbouchet jwstmiriimagerobservationsofsupernovasn1987a
AT rgastaud jwstmiriimagerobservationsofsupernovasn1987a
AT acoulais jwstmiriimagerobservationsofsupernovasn1987a
AT mjbarlow jwstmiriimagerobservationsofsupernovasn1987a
AT cfransson jwstmiriimagerobservationsofsupernovasn1987a
AT pjkavanagh jwstmiriimagerobservationsofsupernovasn1987a
AT jlarsson jwstmiriimagerobservationsofsupernovasn1987a
AT ttemim jwstmiriimagerobservationsofsupernovasn1987a
AT ocjones jwstmiriimagerobservationsofsupernovasn1987a
AT ashirschauer jwstmiriimagerobservationsofsupernovasn1987a
AT ttikkanen jwstmiriimagerobservationsofsupernovasn1987a
AT jadlblommaert jwstmiriimagerobservationsofsupernovasn1987a
AT odfox jwstmiriimagerobservationsofsupernovasn1987a
AT aglasse jwstmiriimagerobservationsofsupernovasn1987a
AT nhabel jwstmiriimagerobservationsofsupernovasn1987a
AT jhjorth jwstmiriimagerobservationsofsupernovasn1987a
AT jjaspers jwstmiriimagerobservationsofsupernovasn1987a
AT okrause jwstmiriimagerobservationsofsupernovasn1987a
AT rmlau jwstmiriimagerobservationsofsupernovasn1987a
AT llenkic jwstmiriimagerobservationsofsupernovasn1987a
AT mmeixner jwstmiriimagerobservationsofsupernovasn1987a
AT onayak jwstmiriimagerobservationsofsupernovasn1987a
AT arest jwstmiriimagerobservationsofsupernovasn1987a
AT bsargent jwstmiriimagerobservationsofsupernovasn1987a
AT rwesson jwstmiriimagerobservationsofsupernovasn1987a
AT gswright jwstmiriimagerobservationsofsupernovasn1987a
AT lcolina jwstmiriimagerobservationsofsupernovasn1987a
AT efvandishoeck jwstmiriimagerobservationsofsupernovasn1987a
AT mgudel jwstmiriimagerobservationsofsupernovasn1987a
AT thhenning jwstmiriimagerobservationsofsupernovasn1987a
AT polagage jwstmiriimagerobservationsofsupernovasn1987a
AT gostlin jwstmiriimagerobservationsofsupernovasn1987a
AT tpray jwstmiriimagerobservationsofsupernovasn1987a
AT bvandenbussche jwstmiriimagerobservationsofsupernovasn1987a