Influence of stellar component on the conditions for thermal instability in the Galactic centre minispiral region

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Previously we demonstrated that collisions between clumps of gas in the circumnuclear disc can reduce their angular momentum and set some of the clumps on a plunging trajectory towards the supermassive black hole. If the central luminosity is determined by the gas accretion mechanism, then there exists a certain range of accretion rate and efﬁciency that allow the thermal instability to sustain the mass inﬂow through the two-temperature medium. Here we explore the stellar component of the nuclear star cluster which acts as an additional source of heating and contributes an additional energy input into the gaseous environment in the Galactic centre Minispiral region.

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