JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip
Dust from core-collapse supernovae (CCSNe), specifically Type IIP supernovae (SNe IIP), has been suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe eject large amounts of newly formed heavy elements, which can condense into dust grains in the cooling ejecta. H...
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2025-01-01
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| author | Melissa Shahbandeh Ori D. Fox Tea Temim Eli Dwek Arkaprabha Sarangi Nathan Smith Luc Dessart Bryony Nickson Michael Engesser Alexei V. Filippenko Thomas G. Brink WeiKang Zheng Tamás Szalai Joel Johansson Armin Rest Schuyler D. Van Dyk Jennifer Andrews Chris Ashall Geoffrey C. Clayton Ilse De Looze James M. DerKacy Michael Dulude Ryan J. Foley Suvi Gezari Sebastian Gomez Shireen Gonzaga Siva Indukuri Jacob Jencson Mansi Kasliwal Zachary G. Lane Ryan Lau David Law Anthony Marston Dan Milisavljevic Richard O’Steen Justin Pierel Matthew Siebert Michael Skrutskie Lou Strolger Samaporn Tinyanont Qinan Wang Brian Williams Lin Xiao Yi Yang Szanna Zsíros |
| author_facet | Melissa Shahbandeh Ori D. Fox Tea Temim Eli Dwek Arkaprabha Sarangi Nathan Smith Luc Dessart Bryony Nickson Michael Engesser Alexei V. Filippenko Thomas G. Brink WeiKang Zheng Tamás Szalai Joel Johansson Armin Rest Schuyler D. Van Dyk Jennifer Andrews Chris Ashall Geoffrey C. Clayton Ilse De Looze James M. DerKacy Michael Dulude Ryan J. Foley Suvi Gezari Sebastian Gomez Shireen Gonzaga Siva Indukuri Jacob Jencson Mansi Kasliwal Zachary G. Lane Ryan Lau David Law Anthony Marston Dan Milisavljevic Richard O’Steen Justin Pierel Matthew Siebert Michael Skrutskie Lou Strolger Samaporn Tinyanont Qinan Wang Brian Williams Lin Xiao Yi Yang Szanna Zsíros |
| author_sort | Melissa Shahbandeh |
| collection | DOAJ |
| description | Dust from core-collapse supernovae (CCSNe), specifically Type IIP supernovae (SNe IIP), has been suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe eject large amounts of newly formed heavy elements, which can condense into dust grains in the cooling ejecta. However, infrared (IR) observations of typical CCSNe generally measure dust masses that are too small to account for the dust production needed at high redshifts. Type IIn SNe (SNe IIn), classified by their dense circumstellar medium, are also known to exhibit strong IR emission from warm dust, but the dust origin and heating mechanism have generally remained unconstrained because of limited observational capabilities in the mid-IR (MIR). Here, we present a JWST/MIRI Medium Resolution Spectrograph spectrum of the SN IIn SN 2005ip nearly 17 yr post-explosion. The SN IIn SN 2005ip is one of the longest-lasting and most well-studied SNe observed to date. Combined with a Spitzer MIR spectrum of SN 2005ip obtained in 2008, this data set provides a rare 15 yr baseline, allowing for a unique investigation of the evolution of dust. The JWST spectrum shows the emergence of an optically thin silicate dust component (≳0.08 M _⊙ ) that is either not present or more compact/optically thick in the earlier Spitzer spectrum. Our analysis shows that this dust is likely newly formed in the cold, dense shell (CDS), between the forward and reverse shocks, and was not preexisting at the time of the explosion. There is also a smaller mass of carbonaceous dust (≳0.005 M _⊙ ) in the ejecta. These observations provide new insights into the role of SN dust production, particularly within the CDS, and its potential contribution to the rapid dust enrichment of the early Universe. |
| format | Article |
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| language | English |
| publishDate | 2025-01-01 |
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| series | The Astrophysical Journal |
| spelling | doaj-art-d47e5d55ed974bd9bb47cf1f33969aaf2025-08-20T03:12:53ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01985226210.3847/1538-4357/adce77JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ipMelissa Shahbandeh0https://orcid.org/0000-0002-9301-5302Ori D. Fox1https://orcid.org/0000-0003-2238-1572Tea Temim2https://orcid.org/0000-0001-7380-3144Eli Dwek3Arkaprabha Sarangi4https://orcid.org/0000-0002-9820-679XNathan Smith5https://orcid.org/0000-0001-5510-2424Luc Dessart6https://orcid.org/0000-0003-0599-8407Bryony Nickson7Michael Engesser8https://orcid.org/0000-0003-0209-674XAlexei V. Filippenko9https://orcid.org/0000-0003-3460-0103Thomas G. Brink10https://orcid.org/0000-0001-5955-2502WeiKang Zheng11https://orcid.org/0000-0002-2636-6508Tamás Szalai12https://orcid.org/0000-0003-4610-1117Joel Johansson13Armin Rest14https://orcid.org/0000-0002-4410-5387Schuyler D. Van Dyk15https://orcid.org/0000-0001-9038-9950Jennifer Andrews16https://orcid.org/0000-0003-0123-0062Chris Ashall17https://orcid.org/0000-0002-5221-7557Geoffrey C. Clayton18https://orcid.org/0000-0002-0141-7436Ilse De Looze19https://orcid.org/0000-0001-9419-6355James M. DerKacy20https://orcid.org/0000-0002-7566-6080Michael Dulude21Ryan J. Foley22https://orcid.org/0000-0002-2445-5275Suvi Gezari23https://orcid.org/0000-0003-3703-5154Sebastian Gomez24https://orcid.org/0000-0001-6395-6702Shireen Gonzaga25Siva Indukuri26Jacob Jencson27https://orcid.org/0000-0001-5754-4007Mansi Kasliwal28https://orcid.org/0000-0002-5619-4938Zachary G. Lane29https://orcid.org/0009-0003-8380-4003Ryan Lau30David Law31https://orcid.org/0000-0002-9402-186XAnthony Marston32https://orcid.org/0000-0001-5788-5258Dan Milisavljevic33https://orcid.org/0000-0002-0763-3885Richard O’Steen34https://orcid.org/0000-0002-2432-8946Justin Pierel35https://orcid.org/0000-0002-2361-7201Matthew Siebert36https://orcid.org/0000-0003-2445-3891Michael Skrutskie37Lou Strolger38https://orcid.org/0000-0002-7756-4440Samaporn Tinyanont39https://orcid.org/0000-0002-1481-4676Qinan Wang40https://orcid.org/0000-0001-5233-6989Brian Williams41https://orcid.org/0000-0003-2063-381XLin Xiao42https://orcid.org/0000-0002-6986-5593Yi Yang43https://orcid.org/0000-0002-6535-8500Szanna Zsíros44https://orcid.org/0000-0001-7473-4208Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduDepartment of Astrophysical Sciences, Princeton University , Princeton, NJ 08544, USAObservational Cosmology Lab, NASA Goddard Space Flight Center , Mail Code 665, Greenbelt, MD 20771, USA; Center for Astrophysics–Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USADARK, Niels Bohr Institute, University of Copenhagen , Jagtvej 155A, 2200 Copenhagen, DenmarkSteward Observatory, University of Arizona , 933 N. Cherry Street, Tucson, AZ 85721, USAInstitut d’Astrophysique de Paris, CNRS-Sorbonne Université , 98 bis boulevard Arago, F-75014 Paris, FranceSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduDepartment of Astronomy, University of California , Berkeley, CA 94720-3411, USADepartment of Astronomy, University of California , Berkeley, CA 94720-3411, USADepartment of Astronomy, University of California , Berkeley, CA 94720-3411, USADepartment of Experimental Physics, Institute of Physics, University of Szeged , H-6720 Szeged, Dóm tér 9, Hungary; MTA-ELTE Lendület “Momentum” Milky Way Research Group , Szent Imre H. st. 112, 9700 Szombathely, HungaryDepartment of Physics, The Oskar Klein Center, Stockholm University , AlbaNova, 10691 Stockholm, SwedenSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.edu; Department of Physics and Astronomy, Johns Hopkins University , 3400 North Charles Street, Baltimore, MD 21218, USACaltech/IPAC , Mailcode 100-22, Pasadena, CA 91125, USAGemini Observatory , 670 N. Aohoku Place, Hilo, HI 96720, USADepartment of Physics, Virginia Tech , Blacksburg, VA 24061, USA; Institute for Astronomy, University of Hawai’i at Manoa , 2680 Woodlawn Drive, Hawai’i, HI 96822, USADepartment of Physics & Astronomy, Louisiana State University , Baton Rouge, LA 70803, USA; Space Science Institute , 4765 Walnut Street, Suite Boulder, CO 80301, USASterrenkundig Observatorium, Ghent University , Krijgslaan 281 - S9, B-9000 Gent, BelgiumSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduDepartment of Astronomy and Astrophysics, University of California , Santa Cruz, CA 95064, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduDepartment of Physics and Astronomy, Johns Hopkins University , 3400 North Charles Street, Baltimore, MD 21218, USAIPAC, Mail Code 100-22, Caltech , 1200 E. California Boulevard, Pasadena, CA 91125, USACahill Center for Astrophysics, California Institute of Technology , 1200 E. California Blvd. Pasadena, CA 91125, USASchool of Physical and Chemical Sciences–Te Kura Matū, University of Canterbury , Private Bag 4800, Christchurch 8140, New ZealandNSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduEuropean Space Agency (ESA) , ESAC, 28692 Villanueva de la Canada, Madrid, SpainPurdue University , Department of Physics and Astronomy, 525 Northwestern Avenue, West Lafayette, IN 4790720, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduDepartment of Astronomy, University of Virginia , Charlottesville, VA 22904-4325, USASpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduNational Astronomical Research Institute of Thailand (NARIT) , Chiang Mai, 50180, ThailandSpace Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218, USA ; mshahbandeh@stsci.eduObservational Cosmology Lab, NASA Goddard Space Flight Center , Code 665, Greenbelt, MD 20771, USADepartment of Physics, College of Physical Sciences and Technology, Hebei University , Baoding 071002, People’s Republic of ChinaDepartment of Astronomy, University of California , Berkeley, CA 94720-3411, USADepartment of Experimental Physics, Institute of Physics, University of Szeged , H-6720 Szeged, Dóm tér 9, HungaryDust from core-collapse supernovae (CCSNe), specifically Type IIP supernovae (SNe IIP), has been suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe eject large amounts of newly formed heavy elements, which can condense into dust grains in the cooling ejecta. However, infrared (IR) observations of typical CCSNe generally measure dust masses that are too small to account for the dust production needed at high redshifts. Type IIn SNe (SNe IIn), classified by their dense circumstellar medium, are also known to exhibit strong IR emission from warm dust, but the dust origin and heating mechanism have generally remained unconstrained because of limited observational capabilities in the mid-IR (MIR). Here, we present a JWST/MIRI Medium Resolution Spectrograph spectrum of the SN IIn SN 2005ip nearly 17 yr post-explosion. The SN IIn SN 2005ip is one of the longest-lasting and most well-studied SNe observed to date. Combined with a Spitzer MIR spectrum of SN 2005ip obtained in 2008, this data set provides a rare 15 yr baseline, allowing for a unique investigation of the evolution of dust. The JWST spectrum shows the emergence of an optically thin silicate dust component (≳0.08 M _⊙ ) that is either not present or more compact/optically thick in the earlier Spitzer spectrum. Our analysis shows that this dust is likely newly formed in the cold, dense shell (CDS), between the forward and reverse shocks, and was not preexisting at the time of the explosion. There is also a smaller mass of carbonaceous dust (≳0.005 M _⊙ ) in the ejecta. These observations provide new insights into the role of SN dust production, particularly within the CDS, and its potential contribution to the rapid dust enrichment of the early Universe.https://doi.org/10.3847/1538-4357/adce77James Webb Space TelescopeInfrared observatoriesCore-collapse supernovaeType II supernovaeSupernovaeAstrophysical dust processes |
| spellingShingle | Melissa Shahbandeh Ori D. Fox Tea Temim Eli Dwek Arkaprabha Sarangi Nathan Smith Luc Dessart Bryony Nickson Michael Engesser Alexei V. Filippenko Thomas G. Brink WeiKang Zheng Tamás Szalai Joel Johansson Armin Rest Schuyler D. Van Dyk Jennifer Andrews Chris Ashall Geoffrey C. Clayton Ilse De Looze James M. DerKacy Michael Dulude Ryan J. Foley Suvi Gezari Sebastian Gomez Shireen Gonzaga Siva Indukuri Jacob Jencson Mansi Kasliwal Zachary G. Lane Ryan Lau David Law Anthony Marston Dan Milisavljevic Richard O’Steen Justin Pierel Matthew Siebert Michael Skrutskie Lou Strolger Samaporn Tinyanont Qinan Wang Brian Williams Lin Xiao Yi Yang Szanna Zsíros JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip The Astrophysical Journal James Webb Space Telescope Infrared observatories Core-collapse supernovae Type II supernovae Supernovae Astrophysical dust processes |
| title | JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip |
| title_full | JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip |
| title_fullStr | JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip |
| title_full_unstemmed | JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip |
| title_short | JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip |
| title_sort | jwst miri observations of newly formed dust in the cold dense shell of the type iin sn 2005ip |
| topic | James Webb Space Telescope Infrared observatories Core-collapse supernovae Type II supernovae Supernovae Astrophysical dust processes |
| url | https://doi.org/10.3847/1538-4357/adce77 |
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