2020
DOI: 10.48550/arxiv.2001.06012
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Positive feedback at the disc-halo interface

Alexander Hobbs,
Robert Feldmann

Abstract: The flat star formation (SF) history of the Milky Way (MW) requires gas in the Galactic disc to be replenished, most likely from a reservoir outside the Galaxy. Such a replenishment may be achieved by a form of 'positive' feedback, whereby SF feedback creates a Galactic fountain cycle that collects and cools additional gas from the hot halo surrounding the Galaxy. In this paper we present a model of this process for the MW. A section of the Galactic disc is allowed to form stars which subsequently explode as s… Show more

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“…However, the gas ejected by SN feedback can cool down at the outskirts of the galaxy and return to the galaxy, a process known as "Galactic fountain" (Shapiro & Field 1976;Bregman 1980;Melioli et al 2008). It is also possible to accomplish such a replenishment in the form of positive SN feedback through which the feedback steals part of the hot gas from the intergalactic medium (IGM) and cools it down to constitute a galactic fountain (Hobbs & Feldmann 2020). These findings suggest that the refurbished cold gas budget may be crucial to sustain SF and black hole feeding, especially in the local Universe.…”
Section: Sfr Vs Bhar and Inferred Luminositiesmentioning
confidence: 99%
“…However, the gas ejected by SN feedback can cool down at the outskirts of the galaxy and return to the galaxy, a process known as "Galactic fountain" (Shapiro & Field 1976;Bregman 1980;Melioli et al 2008). It is also possible to accomplish such a replenishment in the form of positive SN feedback through which the feedback steals part of the hot gas from the intergalactic medium (IGM) and cools it down to constitute a galactic fountain (Hobbs & Feldmann 2020). These findings suggest that the refurbished cold gas budget may be crucial to sustain SF and black hole feeding, especially in the local Universe.…”
Section: Sfr Vs Bhar and Inferred Luminositiesmentioning
confidence: 99%