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In this work, we consider four different galaxy populations and two distinct global environments in the local Universe (z $\leq 0.11$) to investigate the evolution of transitional galaxies (such as star-forming spheroids and passive discs) across dif
Externí odkaz:
http://arxiv.org/abs/2305.08788
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters; Jan2024, Vol. 527 Issue 1, pL19-L25, 7p
