Tootfinder

Rams, Matthew Stafford agree to extension keeping him in L.A. past 2026 https://www.nytimes.com/athletic/7087299/2026/05/21/rams-matthew-stafford-contract-extension/

FW-AUR: Baumkrone droht niederzustürzen Aurich-Extum (ots) - Noch am frühen Sonntagabend musste die Feuerwehr Haxtum zur Beseitigung eines weiteren Sturmschadens ausrücken, der aus dem Unwetter in der Nacht zu Samstag resultierte. In der Extumer Gaste drohte die abgebrochene Krone einer ... https://www.presseportal.de/b…

Die #AfD wittert Alleinregierung. Die Lage der Nation fürchtet zurecht, dass die Juristenbesetzung der frühen 90er bald in Rente geht und Auserwählte nachrücken.
Well, “der Osten” kennt Übernahme: Wessis am Pult, Treuhand, private Windparks als Nachbarn… Siegmund verkauft Übernahme als Befreiung.

@… Interesting read. I actually agree with him, but it's not really a MoCo issue, is it?

South Korea's Hana Bank agrees to acquire a 6.55% stake in Dunamu, which runs South Korea's largest crypto exchange Upbit, for $672.5M from Kakao (Kwanwoo Jun/Wall Street Journal)
https://www.wsj.com/busines…

Star formation powers optical line emission from the CGM
Huanian Zhang, Lizhi Xie, Zhijie Qu, Dennis Zaritsky, Luis C. Ho, Min Bao, Fabio Fontanot, Michaela Hirschmann, Chenxu Liu, Gabriella De Lucia, Enci Wang, Haoyan Zheng
https://arxiv.org/abs/2607.18385 https://arxiv.org/pdf/2607.18385 https://arxiv.org/html/2607.18385
arXiv:2607.18385v1 Announce Type: new
Abstract: Using integral field spectroscopy, we explore the disk-halo interface, or the inner circumgalactic medium (CGM), of individual galaxies by constructing and analyzing emission-line maps for a large sample (72) of normal, low-redshift galaxies spanning three orders of magnitude in stellar mass and four orders in star formation rate (SFR). We find a steep turnover occurring at $(1-2) R_e$ in the H$\alpha$, [O {\small II}], and [O {\small III}] line emission radial profiles. Beyond this radius, the slope of the line emission radial profiles becomes shallower as the SFR of the central galaxy decreases, which might reflect the strength of the feedback processes. The line emission fluxes at large radius ($(5-10) R_e$ or $\sim (0.1-0.25)r_{\rm vir}$) correlate with the galaxy's SFR, but not with its stellar mass. These findings suggest that ionizing photons escaping from star-forming regions in the central galaxy account for the observed emission line fluxes from the inner CGM, with escape fractions inferred from the [O {\small III}] and [O {\small II}] ratio. Different state-of-the-art theoretical models do not agree on the predicted dependence of cool gas on the SFR of the central galaxies, highlighting the importance of CGM emission line measurements to distinguish between different subgrid models for star formation and feedback processes.
toXiv_bot_toot

#RockdenAcker in #Nidderau — wen sehen wir am Samstag um 19:10 Uhr an der Bühne? #DARKK

Poxa, esse time da Suécia tomou gol ršpido da Alemanha agora, hein? 😛
#Copa2026 #CopaFifa2026 #CopaMundialFIFA

O momento chegou! A grande batalha entre os pé-frios! Eu torcendo pra Noruega e Mick Jagger torcendo para a Inglaterra! Quem terš o pé-frio mais poderoso?!!! rs
https://ge.globo.com/futebol/copa-do-m