Tootfinder

Claude is triggered to review all the pull requests that I do to the codebase at work.
While it's working, it's little icon animates like this.
Every time I see it, I imagine it straining to push out it's shit from the chocolate starfish.
Its hard to unsee.
2/3
#ai #claude #graphicDesignIsMyPassion

RIGEL: Feedback regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger
Yunwei Deng, Hui Li, Federico Marinacci, Yang Ni, Boyuan Liu, Aaron Smith, Rahul Kannan, Greg L. Bryan
https://arxiv.org/abs/2510.07368

RIGEL: Feedback regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger
Major mergers of galaxies are likely to trigger bursty star formation activities. The accumulation of dense gas and the boost of star formation efficiency (SFE) are considered to be the two main drivers of the starbursts. However, it is still unclear how each process operates on the scale of individual star-forming clouds. Here, we present a high-resolution (2 Msun) RHD simulation of a gas-rich dwarf galaxy merger using the RIGEL model to investigate how mergers affect the properties of the str…

Sonnet 075 - LXXV
So are you to my thoughts as food to life,
Or as sweet-season'd showers are to the ground;
And for the peace of you I hold such strife
As 'twixt a miser and his wealth is found.
Now proud as an enjoyer, and anon
Doubting the filching age will steal his treasure;
Now counting best to be with you alone,
Then better'd that the world may see my pleasure:
Sometime all full with feasting on your sight,
And by…

Formation and growth of intermediate-mass black holes in dense star clusters: Lessons from N-body and MOCCA Monte Carlo Simulations
Abbas Askar, Marcelo C. Vergara, Sohaib Ali
https://arxiv.org/abs/2510.03766

Formation and growth of intermediate-mass black holes in dense star clusters: Lessons from N-body and MOCCA Monte Carlo Simulations
Dense star clusters are promising nurseries for the formation and growth of intermediate-mass black holes (IMBHs; $\sim 10^2-10^5\,\mathrm{M}_{\odot}$), with increasing observational evidence pointing to their presence in massive star clusters and stripped dwarf-galaxy nuclei. During the early evolution of compact clusters, massive stars can rapidly segregate to the center, where frequent collisions may trigger the runaway growth of a very massive star (VMS). This object can subsequently collap…