Abstract
We have found that the brightest cluster galaxy (BCG) in A85, Holm 15A, displays the largest core known so far. Its cusp radius, r γ = 4.57 ± 0.06 kpc (4.″26 ± 0.″06), is more than 18 times larger than the mean for BCGs and ≳ 1 kpc larger than A2261-BCG, hitherto the largest-cored BCG. Holm 15A hosts the luminous amorphous radio source 0039-095B and has the optical signature of a LINER. Scaling laws indicate that this core could host a supermassive black hole (SMBH) of mass M • ∼ (109-1011) M ⊙. We suggest that cores this large represent a relatively short phase in the evolution of BCGs, whereas the masses of their associated SBMH might be set by initial conditions.
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López-Cruz, O., Añorve, C., Birkinshaw, M., Worrall, D. M., Ibarra-Medel, H. J., Barkhouse, W. A., … Motta, V. (2014). THE BRIGHTEST CLUSTER GALAXY IN A85: The LARGEST CORE KNOWN SO FAR. Astrophysical Journal Letters, 795(2). https://doi.org/10.1088/2041-8205/795/2/L31
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