@astrokiwi For the NEAs in this sample; there are options on thermal fracturing, asymmetric meteoroid bombardment, etc. that would push the rock piles around a little bit without outgassing - Seligman et al. rightly discussed the possibilities at length (comparing to Bennu).
Some may not work - e.g. #1998KY26 spins fast, so thermal swings are low.
But that seems qualitatively different than #ʻOumuamua?
This is really good to see people looking into as it was a key issue with #ʻOumuamua. The level of understanding around low-emission-outgassing minor planets needs to step up a level #astrodon
#TBT to some of the best views of #ʻOumuamua captured from our telescopes. Anything more detailed than this is hypothetical or an artist rendition 😉
This is fig. 1 from @astrokiwi
et al "The Natural History of ‘Oumuamua"