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   	<dc:title>The emergence of Little Red Dots from binary massive black holes</dc:title>
   	<dc:creator>Inayoshi, Kohei</dc:creator>
   	<dc:creator>Shangguan, Jinyi</dc:creator>
   	<dc:creator>Chen, Xian</dc:creator>
   	<dc:creator>Ho, Luis C.</dc:creator>
   	<dc:creator>Haiman, Zoltán ; https://orcid.org/0000-0003-3633-5403</dc:creator>
   	<dc:subject>ddc:520</dc:subject>
   	<dc:description>Little red dots (LRDs) are a newly identified class of broad-line active galactic nuclei (AGNs) with a distinctive V-shaped spectrum characterized by red optical and blue UV continuum emission. Their high abundance at redshifts of z ∼ 6–8 and decline at lower redshifts suggest a transient origin. We propose that the spectral shape of LRDs originates from compact binary black hole systems, in which each black hole is surrounded by a mini-disk and embedded within a larger circumbinary disk. With a binary separation of ≲103 Schwarzschild radii, the Wien tail of a T ≃ 5000 K blackbody spectrum at the inner edge of the circumbinary disk produces the red optical emission, while the mini-disks power the UV continuum. Binary torques carve out a gap between the circumbinary disk and the mini-disks, setting the turnover wavelength of the V-shaped spectrum around the Balmer limit. This scenario naturally reproduces LRD spectra requiring only modest dust attenuation (AV ≲ 1 mag), resolving overestimated luminosities for LRDs in previous studies and alleviating a tension with the so-called Sołtan argument. This model predicts distinct spectral evolution as the binary orbit decays through binary disk interactions and gravitational-wave (GW) emission, linking early-stage “proto-LRD” binaries to the broader AGN population and late-stage “LRD descendants” to coalescing binaries detectable in GW experiments.</dc:description>
   	<dc:publisher>IOP Publishing</dc:publisher>
   	<dc:date>2026</dc:date>
   	<dc:type>info:eu-repo/semantics/article</dc:type>
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   	<dc:type>http://purl.org/coar/resource_type/c_2df8fbb1</dc:type>
   	<dc:identifier>https://research-explorer.ista.ac.at/record/21844</dc:identifier>
   	<dc:identifier>https://research-explorer.ista.ac.at/download/21844/21853</dc:identifier>
   	<dc:source>Inayoshi K, Shangguan J, Chen X, Ho LC, Haiman Z. The emergence of Little Red Dots from binary massive black holes. &lt;i&gt;The Astrophysical Journal&lt;/i&gt;. 2026;1002(1). doi:&lt;a href=&quot;https://doi.org/10.3847/1538-4357/ae548d&quot;&gt;10.3847/1538-4357/ae548d&lt;/a&gt;</dc:source>
   	<dc:language>eng</dc:language>
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   	<dc:relation>info:eu-repo/semantics/altIdentifier/issn/0004-637X</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/e-issn/1538-4357</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/arxiv/2505.05322</dc:relation>
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