A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction

Type Ia supernovae (SNe Ia) arise from the thermonuclear explosions of white dwarfs in multiple-star systems. A rare subclass of SNe Ia exhibit signatures of interaction with circumstellar material (CSM), allowing for direct constraints on companion material. While most known events show evidence fo...

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Main Authors: Geoffrey Mo, Kishalay De, Eli Wiston, Nayana A. J., Raffaella Margutti, Danielle Frostig, Jesper Sollerman, Yashvi Sharma, Takashi J. Moriya, Kevin B. Burdge, Jacob Jencson, Viraj R. Karambelkar, Nathan P. Lourie
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Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/adaf92
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author Geoffrey Mo
Kishalay De
Eli Wiston
Nayana A. J.
Raffaella Margutti
Danielle Frostig
Jesper Sollerman
Yashvi Sharma
Takashi J. Moriya
Kevin B. Burdge
Jacob Jencson
Viraj R. Karambelkar
Nathan P. Lourie
author_facet Geoffrey Mo
Kishalay De
Eli Wiston
Nayana A. J.
Raffaella Margutti
Danielle Frostig
Jesper Sollerman
Yashvi Sharma
Takashi J. Moriya
Kevin B. Burdge
Jacob Jencson
Viraj R. Karambelkar
Nathan P. Lourie
author_sort Geoffrey Mo
collection DOAJ
description Type Ia supernovae (SNe Ia) arise from the thermonuclear explosions of white dwarfs in multiple-star systems. A rare subclass of SNe Ia exhibit signatures of interaction with circumstellar material (CSM), allowing for direct constraints on companion material. While most known events show evidence for dense nearby CSM identified via peak-light spectroscopy (as SNe Ia-CSM), targeted late-time searches have revealed a handful of cases exhibiting delayed CSM interaction with detached shells. Here we present the first all-sky search for late CSM interaction in SNe Ia using a new image subtraction pipeline for mid-infrared data from the NEOWISE space telescope. Analyzing a sample of  ≈8500 SNe Ia, we report evidence for late-time mid-infrared brightening in five previously overlooked events spanning subtypes SNe Iax, SNe Ia-91T, and super-Chandra SNe Ia. Our systematic search doubles the known sample and suggests that ≳0.05% of SNe Ia exhibit mid-infrared signatures of delayed CSM interaction. The mid-infrared light curves ubiquitously indicate the presence of multiple (or extended) detached CSM shells located at ≳10 ^16 –10 ^17 cm, containing 10 ^−6 to 10 ^−4 M _⊙ of dust, with some sources showing evidence for new dust formation, possibly within the cold, dense shell of the ejecta. We do not detect interaction signatures in spectroscopic and radio follow-up; however, the limits are largely consistent with previously confirmed events given the sensitivity and observation phase. Our results highlight that CSM interaction is more prevalent than previously estimated from optical and ultraviolet searches and that mid-infrared synoptic surveys provide a unique window into this phenomenon.
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spelling doaj-art-775d68ea047341dc8f69a4a5e28a77312025-08-20T02:08:49ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019802L3310.3847/2041-8213/adaf92A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar InteractionGeoffrey Mo0https://orcid.org/0000-0001-6331-112XKishalay De1https://orcid.org/0000-0002-8989-0542Eli Wiston2https://orcid.org/0009-0002-4843-2913Nayana A. J.3https://orcid.org/0000-0002-8070-5400Raffaella Margutti4https://orcid.org/0000-0003-4768-7586Danielle Frostig5https://orcid.org/0000-0002-7197-9004Jesper Sollerman6https://orcid.org/0000-0003-1546-6615Yashvi Sharma7https://orcid.org/0000-0003-4531-1745Takashi J. Moriya8https://orcid.org/0000-0003-1169-1954Kevin B. Burdge9https://orcid.org/0000-0002-7226-836XJacob Jencson10https://orcid.org/0000-0001-5754-4007Viraj R. Karambelkar11https://orcid.org/0000-0003-2758-159XNathan P. Lourie12https://orcid.org/0000-0002-4585-9981MIT Kavli Institute for Astrophysics and Space Research , 70 Vassar St., Cambridge, MA 02139, USA ; gmo@mit.eduMIT Kavli Institute for Astrophysics and Space Research , 70 Vassar St., Cambridge, MA 02139, USA ; gmo@mit.eduDepartment of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USADepartment of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USADepartment of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USA; Department of Physics, University of California, Berkeley , 366 Physics North MC 7300, Berkeley, CA 94720, USACenter for Astrophysics ∣ Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USAThe Oskar Klein Centre, Department of Astronomy, Stockholm University , AlbaNova, SE-10691 Stockholm, SwedenDivision of Physics, Mathematics and Astronomy, California Institute of Technology , Pasadena, CA 91125, USANational Astronomical Observatory of Japan, National Institutes of Natural Sciences , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; Graduate Institute for Advanced Studies , SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; School of Physics and Astronomy, Monash University , Clayton, VIC 3800, AustraliaMIT Kavli Institute for Astrophysics and Space Research , 70 Vassar St., Cambridge, MA 02139, USA ; gmo@mit.eduIPAC , Mail Code 100-22, Caltech, 1200 E. California Blvd., Pasadena, CA 91125, USADivision of Physics, Mathematics and Astronomy, California Institute of Technology , Pasadena, CA 91125, USAMIT Kavli Institute for Astrophysics and Space Research , 70 Vassar St., Cambridge, MA 02139, USA ; gmo@mit.eduType Ia supernovae (SNe Ia) arise from the thermonuclear explosions of white dwarfs in multiple-star systems. A rare subclass of SNe Ia exhibit signatures of interaction with circumstellar material (CSM), allowing for direct constraints on companion material. While most known events show evidence for dense nearby CSM identified via peak-light spectroscopy (as SNe Ia-CSM), targeted late-time searches have revealed a handful of cases exhibiting delayed CSM interaction with detached shells. Here we present the first all-sky search for late CSM interaction in SNe Ia using a new image subtraction pipeline for mid-infrared data from the NEOWISE space telescope. Analyzing a sample of  ≈8500 SNe Ia, we report evidence for late-time mid-infrared brightening in five previously overlooked events spanning subtypes SNe Iax, SNe Ia-91T, and super-Chandra SNe Ia. Our systematic search doubles the known sample and suggests that ≳0.05% of SNe Ia exhibit mid-infrared signatures of delayed CSM interaction. The mid-infrared light curves ubiquitously indicate the presence of multiple (or extended) detached CSM shells located at ≳10 ^16 –10 ^17 cm, containing 10 ^−6 to 10 ^−4 M _⊙ of dust, with some sources showing evidence for new dust formation, possibly within the cold, dense shell of the ejecta. We do not detect interaction signatures in spectroscopic and radio follow-up; however, the limits are largely consistent with previously confirmed events given the sensitivity and observation phase. Our results highlight that CSM interaction is more prevalent than previously estimated from optical and ultraviolet searches and that mid-infrared synoptic surveys provide a unique window into this phenomenon.https://doi.org/10.3847/2041-8213/adaf92Type Ia supernovaeInfrared excessSupernovaeCommon envelope binary starsInteracting binary stars
spellingShingle Geoffrey Mo
Kishalay De
Eli Wiston
Nayana A. J.
Raffaella Margutti
Danielle Frostig
Jesper Sollerman
Yashvi Sharma
Takashi J. Moriya
Kevin B. Burdge
Jacob Jencson
Viraj R. Karambelkar
Nathan P. Lourie
A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction
The Astrophysical Journal Letters
Type Ia supernovae
Infrared excess
Supernovae
Common envelope binary stars
Interacting binary stars
title A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction
title_full A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction
title_fullStr A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction
title_full_unstemmed A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction
title_short A Diverse, Overlooked Population of Type Ia Supernovae Exhibiting Mid-infrared Signatures of Delayed Circumstellar Interaction
title_sort diverse overlooked population of type ia supernovae exhibiting mid infrared signatures of delayed circumstellar interaction
topic Type Ia supernovae
Infrared excess
Supernovae
Common envelope binary stars
Interacting binary stars
url https://doi.org/10.3847/2041-8213/adaf92
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