2019
Spitzer mid-infrared detections of neutron star merger GW170817 suggests synthesis of the heaviest elements
Abstract: We report our Spitzer Space Telescope observations and detections of the binary neutron star merger GW170817. At 4.5µm, GW170817 is detected at 21.9 mag AB at +43 days and 23.9 mag AB at +74 days after merger. At 3.6µm, GW170817 is not detected to a limit of 23.2 mag AB at +43 days and 23.1 mag AB at +74 days. Our detections constitute the latest and reddest constraints on the kilonova/macronova emission and composition of heavy elements. The 4.5µm luminosity at this late phase cannot be explained by elements …
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Cited by 124 publications
(91 citation statements)
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“…27 . Furthermore, the late-time mid-infrared emission and colours are consistent with those observed with AT2017gfo with Spitzer 24 . These similarities further strengthen both the kilonova interpretation and the redshift measurement of GRB 230307A (Fig.…”
Section: Mainsupporting
confidence: 84%
“…27 . Furthermore, the late-time mid-infrared emission and colours are consistent with those observed with AT2017gfo with Spitzer 24 . These similarities further strengthen both the kilonova interpretation and the redshift measurement of GRB 230307A (Fig.…”
Section: Mainsupporting
confidence: 84%
“…We assume the radioactivity of 𝑟-process nuclei as the source of heat and ionization. Note that the light curve of the GW170817 kilonova is consistent with the picture that 𝛽-decay of 𝑟-process nuclei predominantly heats the ejecta material over the time scales from 0.5 to 70 day (e.g., Kasliwal et al 2019) 1 . In the nebular phase, the ejecta is optically thin for 𝛾-rays, and hence, we consider only 𝛽-decay electrons.…”
Section: Time Scale Radioactive Heat and Ionizationsupporting
confidence: 79%
“…The red line shows the simple power-law heating q ∼ 10 10 erg g −1 s −1 (t/1 day) −1.3 . The black dot with an error bar is the heating rate at t=43 day obtained by Kasliwal et al (2019) using the mid-infrared observations by Spitzer, which are consistent with the heating rates shown by the red lines. Since the current X-ray light curve suggests the super-Eddington phase, the halting time has not likely been reached yet.…”
Section: X-ray Light Curve Of the Fallback Accretion In Bns Mergersupporting
confidence: 78%
