Stellar collisions in flattened and rotating Population III star clusters

Fragmentation often occurs in disk-like structures, both in the early Universe and in the context of present-day star formation. Supermassive black holes (SMBHs) are astrophysical objects whose origin is not well understood; they weigh millions of solar masses and reside in the centers of galaxies....

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-05, Vol.649, p.A160
Hauptverfasser:	Vergara, M. Z. C., Schleicher, D. R. G., Boekholt, T. C. N., Reinoso, B., Fellhauer, M., Klessen, R. S., Leigh, N. W. C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Collision rates Galactic evolution Massive stars Population III stars Scale height Space telescopes Star & galaxy formation Star clusters Star formation Star mergers Stellar evolution Stellar rotation Stellar winds Supermassive black holes
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