{"paper":{"title":"Supermassive Black Holes and Nuclear Star Clusters: Connection with the Host Galaxy Kinematics and Color","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A.M. Cherepashchuk (Lomonosov Moscow State University, A.V. Zasov, Moscow, Russia), Sternberg Astronomical Institute","submitted_at":"2013-12-16T06:28:51Z","abstract_excerpt":"We consider the relationship between the masses of the central objects in disky galaxies - supermassive black holes (SMBHs) and nuclear star clusters (NCs) - and various parameters of parent galaxies: velocity of rotation $V_{(2)}$ at $R= 2$ kpc, maximal velocity of rotation $V_{\\textrm{max}}$, the indicative dynamical mass $M_{25}$, the total mass of the stellar population $M_{*}$, and the total color index ($B{-}V$). The mass of nuclear clusters $M_{\\rm nc}$ correlates more closely with the kinematic parameters and total mass of galaxies than the mass of central black holes $M_{\\rm bh}$, inc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.4255","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}