The spatially offset quasar E1821+643: new evidence for gravitational recoil
Date Issued
2021
Author(s)
Abstract
A galaxy merger is expected to cause the formation of a supermassive black hole (SMBH) binary, which itself eventually coalesces through the anisotropic emission of gravitational waves. This may result in the merged SMBH receiving a recoil kick velocity ~100-1000 kms-1, causing it to oscillate in the gravitational potential of the host galaxy. The luminous quasar E1821+643, identified as an SMBH recoil candidate via spectropolarimetry observations, shows Doppler shifting of the broad emission lines in direct and scattered light, consistent with a relative velocity of 2100 km s-1 between the quasar nucleus and host galaxy. In this paper, we attempt to detect the expected spatial displacement using a combination of optical spectroastrometry and Hubble Space Telescope (HST) narrow-band images. The spectroastrometry reveals a relative spatial displacement between the quasar nucleus and the gas emitting the [O III] λλ4959, 5007 lines of ~130 mas (~580 pc) to the north-west. Our HST images resolve the [O III] emission on sub-arcsecond scales, showing that it is asymmetrically distributed, extending to radial distances ~0.5-0.6 arcsec from the nucleus in a wide arc running from the north-east around to the west. A simulated spectroastrometry observation based on the HST [O III] image indicates that only a small fraction of the measured displacement can be attributed to the asymmetric [O III] emission. This displacement therefore appears to be a real spatial offset of the quasar nucleus with respect to the narrow-line region, presumed to be located at the host galaxy centre, further supporting the interpretation that a post-merger gravitational recoil of the SMBH has occurred in E1821+643.
Volume
507
Issue
1
Start page
484
Issn Identifier
0035-8711
Ads BibCode
2021MNRAS.507..484J
Rights
open.access
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