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It is thought that even in our own galaxy, mergers of old low metallicity stars may form massive stars capable of creating a pair instability supernova.
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Others form massive and shapeless or leaflike growths.
Towards the end of their evolution, massive stars form massive (∼1.5 solar mass) iron cores at their center.
To create a supermassive black hole, you first have to form massive stars.
Finally, super-massive stars with ({simeq}10^{5}mbox10^{6}mbox { M}_{odot}) may form in atomic cooling halos in which previous star formation was suppressed.
Here, we focus on the interaction of light rays with the strong gravitational field of a massive black hole and show that relativistic images may form.
These super AGB stars may form the majority of core collapse supernovae, although less luminous and so less commonly observed than those from more massive progenitors.
Divisive rival camps may form.
A few females may form spinster herds.
Sometimes, wetlands may form.
These may form your core group.
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