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• W2035739464 startingPage "L6" @default.
• W2035739464 abstract "A growing number of observations reveal a subset of Type Ia supernovae undergoing circumstellar interaction (SNe Ia-CSM). We present unpublished archival Spitzer Space Telescope data on SNe Ia-CSM 2002ic and 2005gj obtained > 1300 and 500 days post-discovery, respectively. Both SNe show evidence for late-time mid-infrared (mid-IR) emission from warm dust. The dust parameters are most consistent with a pre-existing dust shell that lies beyond the forward-shock radius, most likely radiatively heated by optical and X-ray emission continuously generated by late-time CSM interaction. In the case of SN 2005gj, the mid-IR luminosity more than doubles after 1 year post-discovery. While we are not aware of any late-time optical-wavelength observations at these epochs, we attribute this rebrightening to renewed shock interaction with a dense circumstellar shell." @default.
• W2035739464 created "2016-06-24" @default.
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• W2035739464 date "2013-07-05" @default.
• W2035739464 modified "2023-09-25" @default.
• W2035739464 title "THE LATE-TIME REBRIGHTENING OF TYPE Ia SN 2005gj IN THE MID-INFRARED" @default.
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• W2035739464 doi "https://doi.org/10.1088/2041-8205/772/1/l6" @default.
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