  Recent studies of high-redshift galaxies with James Webb Space Telescope
(JWST), such as GN-z11 at $z=10.6,$ show unexpectedly significant amounts of
nitrogen (N) in their spectra. As this phenomenology appears to extend to
gravitionally lensed galaxies at Cosmic noon such as the Sunburst Arc at
$z=2.37$, as well as globular clusters overall, we suggest that the common
ingredient among them are very massive stars (VMSs) with zero-age main sequence
(ZAMS) masses in the range of 100-1000 $M_{\odot}$. The He II in the Sunburst
Arc might also be the result of the disproportionally large contribution of VMS
to the total stellar contribution. We analyse the pros and cons of the previous
suggestions, including classical Wolf-Rayet (cWR) stars and supermassive stars
(SMSs), to conclude that only our VMS alternative ticks all the relevant boxes.
We discuss the VMS mass-loss history via their peculiar vertical evolution in
the HR diagram resulting from a self-regulatory effect of these wind-dominated
VMSs and we estimate that the large amounts of N present in star-forming
galaxies may indeed result from VMSs. We conclude that VMSs should be included
in population synthesis and chemical evolution models. Moreover, that it is
critical for this to be done self-consistently, as a small error in their
mass-loss rates would have dramatic consequences for their stellar evolution,
as well as their ionising and chemical feedback.
