International audience; We revisit motility-induced phase separation in two models of active particles interacting by pair-wise repulsion. We show that the resulting dense phase contains gas bubbles distributed algebraically up to a typically large cutoff scale. At large enough system size and/or global density, all the gas may be contained inside the bubbles, at which point the system is microphase-separated with a finite cutoff bubble scale. We observe that the ordering is anomalous, with different dynamics for the coarsening of the dense phase and of the gas bubbles. This phenomenology is reproduced by a "reduced bubble model" that implements the basic idea of reverse Ostwald ripening put forward in Tjhung et al. [Phys. Rev. X 8, 031080 (2018)]. Self-propelled particles interacting solely with steric repulsion are well known to be able to spontaneously separate into a macroscopic dense cluster and a residual gas, in spite of the absence of explicit attraction forces. This motility-induced phase separation (MIPS) [1] of active particles has become a cornerstone of the physics of dry active matter (in which the fluid surrounding particles is neglected). As such, it has driven many theoretical works [2-7] as well as countless numerical studies (see, e.g. [8-15] to name a few prominent ones). The motil-ity reduction resulting from persistent collisions, which leads to MIPS, is a generic ingredient encountered both in living and synthetic active matter [16-19]. Despite its purely non-equilibrium origin, MIPS was initially described as a conventional phase separation between two homogeneous macroscopic phases. It was first predicted in models of quorum-sensing particles [2] where particle speed decreases with the local density, without two-body interactions. In this case, equilibrium-like thermodynamics can be constructed to account quantitatively for phase coexistence [20]. For systems of repulsive disks, attempts were made to model the speed reduction due to collisions by a quorum-sensing interaction [3, 8, 10], but the results are not satisfactory, due to fundamental differences between the two cases [5, 21]. There is indeed mounting evidence that more complex physics is at play in systems of repulsive disks. In particular , the surface tension between the dense phase and the gas, defined via the Laplace law, has been measured to be negative [20, 22, 23], triggering a spate of controversy[24]. This was rationalized at field theoretical level by including terms that break detailed balance in the classical theory for equilibrium liquid-gas phase separation. In this active Model B+ (AMB+), surface tension can become negative for some parameter values, in which case Ost-wald ripening is reversed for vapor bubbles while still remaining normal for liquid droplets. This means that small vapor bubbles, contrary to the standard scenario, grow at the expense of larger ones due to a diffusion flux. When this happens, simulations of AMB+ lead to either a bubbly fluid interpreted as microphase separation, or to the coexistence of a dense phase populated of bubbles with an outer gas [7]. There is in fact incidental evidence for such a bubbly liquid at particle level [9, 11, 12, 20, 22], but it has not yet been studied per se. Very recently, Ca-porusso et al [25] have shown more clearly that in systems with hard-core interactions, the dense phase is made of hexatic subdomains and interstitial gas regions. In this Letter we show, within two standard particle models displaying MIPS, that not only the dense phase is endowed with bubbles, but also that these are distributed algebraically up to some cutoff scale that we observe to grow with system size. Finite-size scaling based on this observation suggests that, as system size increases, more and more of the gas is contained in bubbles. At large densities, we are able to observe the vanishing of the macroscopic gas reservoir, and the system is then microphase-separated with bubbles of all sizes up to a maximal bubble size that depends on the average density. Moreover, the coarsening of bubbles is anomalous with the typical length scale growing as t 0.22. We elucidate the basic mechanisms at play, and show, within a reduced model implementing reversed Ostwald ripening for gas bubbles, that they indeed lead to a self-organized critical dynamics. Self-organized critical phase coexistence. We first consider the paradigmatic active brownian particles (ABPs) introduced in [8]. Self-propelled by a force of constant magnitude F 0 along its internal polarity u i = (cos θ i , sin θ i), particle i evolves according to the over-damped Langevin equations governing its position r i and polar angle θ i : r i = µ i (F 0 u i + F i) + η i ;θ i = η i (1) where F i = − j =i ∇V (r i − r j) is the force exerted on particle i by the other particles. We choose the pair potential to be a short-range harmonic repulsion V (r) = k 2 (σ − r) 2 if r < σ and 0 otherwise with k the arXiv:2007.03587v1 [cond-mat.stat-mech] 7 Jul 2020