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Deep Galaxy Stellar Mass Functions As a Function of Star Formation Rate in the Virgo Cluster Environment

We analyze deep ( M _* ≳ 10 ^7 M _⊙ ) galaxy stellar mass functions (SMFs) of the Virgo cluster using stellar masses derived as part of the Next Generation Virgo Survey. The total SMF has a slope of $\alpha =-1.3{5}_{-0.02}^{+0.02}$ , which is similar to or steeper than typical field values. Using d...

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Bibliografiset tiedot
Päätekijät: Cameron R. Morgan, Elizaveta Sazonova, Ian D. Roberts, Michael L. Balogh, Joel Roediger, Laura Ferrarese, Patrick Côté, Alessandro Boselli, Matteo Fossati, Jean-Charles Cuillandre, Stephen Gwyn
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astrophysical Journal
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Linkit:https://doi.org/10.3847/1538-4357/addc6c
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