paper

SDSS J125417.98+274004.6: An X-ray Detected Minor Merger Dual AGN

arXiv:2310.09945 · doi:10.21105/astro.2310.09945

Abstract

In this paper, we present the discovery of a dual AGN in a 11:1 minor merger between the galaxy SDSS J125417.98+274004.6 and its unnamed dwarf satellite. We calculated stellar masses of the primary and secondary galaxy to be 2.510M and 2.210M, respectively. We used archival Chandra X-ray observations to assess the presence of AGN. We found that both AGN have comparable luminosities of 210 erg s, with the secondary AGN being more likely to be the dominant one. The galaxies are in the early stages of the merger and are connected by a tidal bridge. Previous works suggest that the secondary AGN should experience a brief but intensive period of Eddington-limit approaching accretion during the early stages of the merger. During the merger, the secondary black hole can increase its mass by a factor of ten. SDSS J125417.98+274004.6 is the first known dual AGN in an early-stage minor merger with a comparably or more luminous secondary AGN. As such, it will be of great value for future studies of merger-triggered accretion and black hole growth mechanisms.

6 pages, 3 figures, 2 tables. Accepted for publication in the Open Journal of Astrophysics

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