Top Tweets for #SS4MS
K. (Wren) Suess: Post-starbursts can contain significant molecular gas! But it seems to disappear on short timescale since quenching - just 85 Myr! (Bezanson+22)
Does gas become less dense and escape CO detection? #SS4MS #EAS2022 #EASValencia2022

U. Kuchner summarises mixed results on how galaxies living in/around filaments are affected by them.
Challenge: How to define a multi-structure filament?
This could help to explain the observed diversity around the MS. #SS4MS #EAS2022 #EASValencia2022

C. de Sá Freitas summarises how different quenching processes (with different timescales) are linked to morphology in SDSS #SS4MS #EAS2022 #EASValencia2022

S. Tacchella illustrating how different spatial scales and timescales all come into play when looking at processes affecting star formation in galaxies #SS4MS #EAS2022 #EASValencia2022

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