Keck/ESI Long-slit Spectroscopy of SBS 1421+511: A Recoiling Quasar Nucleus in An Active Galaxy Pair?

TL;DR

This study uses Keck/ESI spectroscopy to analyze SBS 1421+511, revealing a potential recoiling black hole in an interacting galaxy pair with dual AGN features and complex emission line structures.

Contribution

It provides evidence supporting a recoiling active black hole scenario and characterizes the galaxy pair as likely hosting dual AGN with extended emission regions.

Findings

The quasar exhibits a blueshifted broad emission line profile consistent with a recoiling black hole.

The extended source shows Seyfert-like narrow lines and is at a similar redshift, indicating an interacting galaxy pair.

Extended emission lines suggest tidal interactions or outflows related to the quasar activity.

Abstract

We present Keck/ESI long-slit spectroscopy of SBS 1421+511, a system consisting of a quasar at z = 0.276 and an extended source 3" northern to the quasar. The quasar shows a blue-skewed profile of Balmer broad emission lines, which can be well modeled as emissions from a circular disk with a blueshift velocity of ~1400 km/s. The blueshift is better interpreted as resulting from a recoiling active black hole than from a super-massive black hole binary, since the line profile almost kept steady over one decade in the quasar rest-frame. Alternative interpretations are possible as well, such as emissions from a bipolar outflow or a circular disk with spiral emissivity perturbations. The extended source shows Seyfert-like narrow line ratios and a [OIII] luminosity of >1.4\times10^8L_\odot, with almost the same redshift as the quasar and a projected distance of 12.5 kpc at the redshift. SBS 1421+511 is thus likely to be an interacting galaxy pair with dual AGN. Alternatively, the quasar companion only appears to be active but not necessarily so: the gas before/in/behind the companion galaxy is illuminated by the quasar as an extended emission line region is detected at a similar distance in the opposite direction southern to the quasar, which may be generated either by tidal interactions between the galaxy pair or large-scale outflows from the quasar.