JWST MIRI Imager Observations of Supernova SN 1987A

被引：0

作者：

Bouchet, P. ^{[1
]}

Gastaud, R. ^{[2
]}

Coulais, A. ^{[1
,3
]}

Barlow, M. J. ^{[4
]}

Fransson, C. ^{[5
]}

Kavanagh, P. J. ^{[6
,7
]}

Larsson, J. ^{[8
]}

Temim, T. ^{[9
]}

Jones, O. C. ^{[10
]}

Hirschauer, A. S. ^{[11
]}

Tikkanen, T. ^{[12
]}

Blommaert, J. A. D. L. ^{[13
]}

Fox, O. D. ^{[11
]}

Glasse, A. ^{[10
]}

Habel, N. ^{[14
]}

Hjorth, J. ^{[15
]}

Jaspers, J. ^{[6
,7
]}

Krause, O. ^{[16
]}

Lau, R. M. ^{[17
]}

Lenkic, L. ^{[14
]}

Meixner, M. ^{[18
]}

Nayak, O. ^{[11
]}

Rest, A. ^{[11
,19
]}

Sargent, B. ^{[11
,20
]}

Wesson, R. ^{[21
]}

Wright, G. S. ^{[10
]}

Colina, L. ^{[22
]}

van Dishoeck, E. F. ^{[23
,24
]}

Guedel, M. ^{[25
,26
,27
]}

Henning, Th. ^{[23
]}

Lagage, P. -o. ^{[1
]}

Oestlin, G. ^{[5
]}

Ray, T. P. ^{[7
]}

Vandenbussche, B. ^{[28
]}

机构：

[1] Univ Paris Saclay, Univ Paris Cite, CEA, CNRS, F-91191 Gif Sur Yvette, France

[2] Univ Paris Saclay, CEA, DEDIP, F-91191 Gif Sur Yvette, France

[3] Univ PSL, Sorbonne Univ, LERMA, Observ Paris, Paris, France

[4] Univ Coll London UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[5] Stockholm Univ, Oskar Klein Ctr, Dept Astron, AlbaNova, SE-10691 Stockholm, Sweden

[6] Maynooth Univ, Dept Expt Phys, Irelan, Maynooth, Co Kildare, Ireland

[7] Dublin Inst Adv Studies, Sch Cosm Phys, Astron & Astrophys Sect, 31 Fitzwilliam Pl, Dublin, Ireland

[8] KTH Royal Inst Technol, Oskar Klein Ctr, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden

[9] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[10] UK Astron Technol Ctr, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Scotland

[11] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[12] Univ Leicester, Space Res Ctr, Sch Phys & Astron, Space Pk Leicester,92 Corp Rd, Leicester LE4 5SP, England

[13] Vrije Univ Brussel, Dept Phys & Astrophys, Astron & Astrophys Res Grp, Pleinlaan 2, B-1050 Brussels, Belgium

[14] NASA Ames Res Ctr, Stratospher Observ Infrared Astron, Mail Stop 204-14, Moffett Field, CA 94035 USA

[15] Univ Copenhagen, Niels Bohr Inst, DARK, Jagtvej 128, DK-2200 Copenhagen, Denmark

[16] Max Planck Inst Astron, Heidelberg MPIA, Heidelberg, Germany

[17] NSFs NOIR Lab, 950 Cherry Ave, Tucson, AZ 85721 USA

[18] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[19] Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA

[20] Johns Hopkins Univ, Ctr Astrophys Sci, William H Miller Dept Phys & Astron 3, Baltimore, MD 21218 USA

[21] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, Wales

[22] Ctr Astrobiol CAB, CSIC INTA, Ctra Ajalvir Km 4, E-28850 Torrejon De Ardoz, Madrid, Spain

[23] Max Planck Inst Extraterresstr Phys MPE, Giessenbachstr 1, D-85748 Garching, Germany

[24] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[25] Univ Vienna, Dept Astrophys, Turkenschanzstr 17, A-1180 Vienna, Austria

[26] Max Planck Inst Astron MPIA, Konigstuhl 17, D-69117 Heidelberg, Germany

[27] Inst Particle Phys & Astrophys, ETH Zurich, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland

[28] Inst Astron, KU Leuwen, Celestijnenlaan 200D, B-3001 Leuwen, Belgium

来源：

ASTROPHYSICAL JOURNAL | 2024年 / 965卷 / 01期

基金：

美国国家航空航天局; 爱尔兰科学基金会; 英国科学技术设施理事会; 欧洲研究理事会;

关键词：

WEBB-SPACE-TELESCOPE; RADIO REMNANT; MIDINFRARED INSTRUMENT; CIRCUMSTELLAR RING; COMPACT OBJECT; BLAST WAVE; EJECTA; DUST; EVOLUTION; SN-1987A;

D O I：

10.3847/1538-4357/ad2770

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：15

共 50 条

[41] CHEMISTRY IN SUPERNOVA 1987A
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[42] ULTRAVIOLET OBSERVATIONS OF SN 1987A WITH THE IUE SATELLITE
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[44] REVIEW OF SUPERNOVA 1987A
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[47] Bayesian analysis of neutrinos observed from supernova SN 1987A
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[50] SPECKLE INTERFEROMETRIC OBSERVATIONS OF SUPERNOVA 1987A AND OF A BRIGHT ASSOCIATED SOURCE
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