An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients
Journal
Date Issued
2019
Author(s)
Margutti, R.
•
Metzger, B. D.
•
Chornock, R.
•
Vurm, I.
•
Roth, N.
•
Grefenstette, B. W.
•
Savchenko, V.
•
Cartier, R.
•
Steiner, J. F.
•
Terreran, G.
•
Margalit, B.
•
•
Milisavljevic, D.
•
Alexander, K. D.
•
Bietenholz, M.
•
Blanchard, P. K.
•
Bozzo, E.
•
Brethauer, D.
•
Chilingarian, I. V.
•
Coppejans, D. L.
•
Ducci, L.
•
Ferrigno, C.
•
Fong, W.
•
Götz, D.
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Guidorzi, C.
•
Hajela, A.
•
Hurley, K.
•
Kuulkers, E.
•
Laurent, P.
•
•
Nicholl, M.
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Patnaude, D.
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Ubertini, P.
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Banovetz, J.
•
Bartel, N.
•
Berger, E.
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Coughlin, E. R.
•
Eftekhari, T.
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Frederiks, D. D.
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Kozlova, A. V.
•
Laskar, T.
•
Svinkin, D. S.
•
Drout, M. R.
•
MacFadyen, A.
•
Paterson, K.
Abstract
We present the first extensive radio to γ-ray observations of a fast-rising blue optical transient, AT 2018cow, over its first ∼100 days. AT 2018cow rose over a few days to a peak luminosity L pk ∼ 4 × 1044 erg s-1, exceeding that of superluminous supernovae (SNe), before declining as L ∝ t -2. Initial spectra at δt ≲ 15 days were mostly featureless and indicated large expansion velocities v ∼ 0.1c and temperatures reaching T ∼ 3 × 104 K. Later spectra revealed a persistent optically thick photosphere and the emergence of H and He emission features with v ∼ 4000 km s-1 with no evidence for ejecta cooling. Our broadband monitoring revealed a hard X-ray spectral component at E ≥ 10 keV, in addition to luminous and highly variable soft X-rays, with properties unprecedented among astronomical transients. An abrupt change in the X-ray decay rate and variability appears to accompany the change in optical spectral properties. AT 2018cow showed bright radio emission consistent with the interaction of a blast wave with v sh ∼ 0.1c with a dense environment (\dot{M}∼ {10}-3-{10}-4 {M}☉ {yr}}-1 for v w = 1000 km s-1). While these properties exclude 56Ni-powered transients, our multiwavelength analysis instead indicates that AT 2018cow harbored a “central engine,” either a compact object (magnetar or black hole) or an embedded internal shock produced by interaction with a compact, dense circumstellar medium. The engine released ∼1050-1051.5 erg over ∼103-105 s and resides within low-mass fast-moving material with equatorial-polar density asymmetry (M ej,fast ≲ 0.3 M ☉). Successful SNe from low-mass H-rich stars (like electron-capture SNe) or failed explosions from blue supergiants satisfy these constraints. Intermediate-mass black holes are disfavored by the large environmental density probed by the radio observations.
Volume
872
Issue
1
Start page
18
Issn Identifier
0004-637X
Ads BibCode
2019ApJ...872...18M
Rights
open.access
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