Where is the Engine Hiding Its Missing Energy? Constraints from a Deep X-Ray Non-detection of the Superluminous SN 2015bn

Kornpob Bhirombhakdi, Ryan Chornock, Raffaella Margutti, Matt Nicholl, Brian D. Metzger, Edo Berger, Ben Margalit, Dan Milisavljevic

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

SN 2015bn is a nearby hydrogen-poor superluminous supernova (SLSN-I) that has been intensively observed in X-rays with the goal to detect the spindown powered emission from a magnetar engine. The early-time ultraviolet/optical/infrared (UVOIR) data fit well to the magnetar model, but require leakage of energy at late times of ≲1043 erg s-1, which is expected to be partially emitted in X-rays. Deep X-ray limits until ∼300 days after explosion revealed no X-ray emission. Here, we present the latest deep 0.3-10 keV X-ray limit at 805 days obtained with XMM-Newton. We find L X < 1041 erg s-1, with no direct evidence for central-engine powered emission. While the late-time optical data still follow the prediction of the magnetar model, the best-fit model to the bolometric light curve predicts that ∼97% of the total input luminosity of the magnetar is escaping outside of the UVOIR bandpass at the time of observation. Our X-ray upper limit is <1.5% of the input luminosity, strongly constraining the high-energy leakage, unless non-radiative losses are important. These deep X-ray observations identify a missing energy problem in SLSNe-I, and we suggest future observations in hard X-rays and γ-rays for better constraints. Also, independent of the optical data, we constrain the parameter spaces of various X-ray emission scenarios, including ionization breakout by magnetar spindown, shock interaction between the ejecta and external circumstellar medium, off-axis γ-ray burst afterglow, and black hole fallback accretion.

Original languageEnglish (US)
Article numberL32
JournalAstrophysical Journal Letters
Volume868
Issue number2
DOIs
StatePublished - Dec 1 2018

Keywords

  • X-rays: individual (SN 2015bn)
  • supernovae: individual (SN 2015bn)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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