Tootfinder

done a bit of sprucing to the football nook, finally put my scarves up and put up the new shirts I got specifically for decoration (bc they don't fit me lol)
I need to acquire a ladder or a tall friend to fill in the space higher up #fedifc

Why isn't it possible to simply agree that we must do 2 things to mitigate #climate change: 1) Eliminate nearly all anthropogenic GHG emissions and 2) Increase the rate of CO2 sequestration?
And then we can focus on the merits/demerits of actions in both spaces? We are not facing exclusive options here, after all. (1/2)
Could nature itself hold the solution to climate change?

Why isn't it possible to simply agree that we must do 2 things to mitigate #climate change: 1) Eliminate nearly all anthropogenic GHG emissions and 2) Increase the rate of CO2 sequestration?
And then we can focus on the merits/demerits of actions in both spaces? We are not facing exclusive options here, after all. (1/2)
Could nature itself hold the solution to climate change?

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

Ajer is late on a great pass and VAR finds it a penalty. I thought so live, although I thought Ajer got a tiny piece of the ball.
SAVED! Feels like justice to me.
#BRAPAR #WorldCup #fedifc