AK
Albrecht W. H. Kamlah
astro-ph.GAastro-ph.SRastro-ph.HEastro-ph.COastro-ph.IMgr-qc
On Valency
published · living versionsW_g4ngvay5·v1 · currentpublished
The STARfall pathway: forging intermediate-mass black holes through stellar collisions in dense star clusters
with Filippo Simonato, Manuel Arca Sedda, Taeho Ryu, Jakub Klencki +13
1 version
Preprints & journals
12 papers in the corpus · 2021–2026Direct N-body simulations of rotating and extremely massive Population III star clusters2603.29657v2 · Kai Wu, Ataru Tanikawa, Francesco Flammini Dotti et al.2026 · 1 citationA&A 709, A142 (2026)
Evolution of star clusters with initial bulk rotation via N-body simulations2505.20432v4 · Abylay Bissekenov, Xiaoying Pang, Albrecht Kamlah et al.2025 · 6 citationsA&A 699, A196 (2025)
Rapid formation of a very massive star >50000 and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters2505.07491v2 · Marcelo C. Vergara, Abbas Askar, Albrecht W. H. Kamlah et al.2025 · 20 citationsA&A 704, A321 (2025)
Efficiency of black hole formation via collisions in stellar systems: An analysis of data from simulations and observations2405.12008v2 · M.C. Vergara, D.R.G. Schleicher, A. Escala et al.2024 · 16 citationsA&A 689, A34 (2024)
Growth of Seed Black Holes in Galactic Nuclei2307.08068v1 · Rainer Spurzem, Francesco Rizzuto, Manuel Arca Sedda et al.2023 · 1 citationIn: NIC Symposium 2022, M.M\"uller, Ch. Peter, A. Trautmann (Editors), ISBN 978-3-95806-646-5 (Book), DNB Link for this article: https://d-nb.info/1286760135
The Dragon-II simulations -- I. Evolution of single and binary compact objects in star clusters with up to 1 million stars2307.04805v1 · Manuel Arca Sedda, Albrecht W. H. Kamlah, Rainer Spurzem et al.2023 · 42 citationsarXiv
The Dragon-II simulations -- II. Formation mechanisms, mass, and spin of intermediate-mass black holes in star clusters with up to 1 million stars2307.04806v1 · Manuel Arca Sedda, Albrecht W. H. Kamlah, Rainer Spurzem et al.2023 · 54 citationsarXiv
The Dragon-II simulations -- III. Compact binary mergers in clusters with up to 1 million stars: mass, spin, eccentricity, merger rate and pair instability supernovae rate2307.04807v1 · Manuel Arca Sedda, Albrecht W. H. Kamlah, Rainer Spurzem et al.2023 · 37 citationsarXiv
Computational Methods for Collisional Stellar Systems2305.11606v1 · Rainer Spurzem, Albrecht Kamlah2023 · 25 citationsarXiv
PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 6282211.13997v2 · Nils Hoyer, Francesca Pinna, Albrecht W. H. Kamlah et al.2022 · 16 citationsarXiv
The impact of stellar evolution on rotating star clusters: the gravothermal-gravogyro catastrophe and the formation of a bar of black holes2205.04470v2 · A. W. H. Kamlah, R. Spurzem, P. Berczik et al.2022 · 40 citationsarXiv
Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster2105.08067v2 · A. W. H. Kamlah, A. Leveque, R. Spurzem et al.2021 · 74 citationsarXiv
Career total: 21 works. 12 are in this corpus.
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