• Corpus ID: 231986069

Capturing the inside-out quenching by black holes with far-infrared atomic line ratios

@inproceedings{Inoue2021CapturingTI,
  title={Capturing the inside-out quenching by black holes with far-infrared atomic line ratios},
  author={Shigeki Inoue and Hiroshi Matsuo and Naoki Yoshida and Hidenobu Yajima and Kana Moriwaki},
  year={2021}
}
We propose to use relative strengths of far-infrared fine structure lines from galaxies to characterise early phases of the inside-out quenching by massive black holes (BHs). The BH feedback is thought to quench star formation by evacuating the ambient gas. In order to quantify the feedback effect on the gas density in the galactic centres, we utilise the outputs of IllustrisTNG and Illustris simulations, which implement different BH feedback models. We devise a physical model of H II regions… 

References

SHOWING 1-4 OF 4 REFERENCES
The initial mass function 50 years later
Preface,List of Participants,Part I The IMF Concept through Time, Introduction to IMF@50, Ed, me, and the Insterstellar Medium,The IMF challenge - 25 questions, Fifty years of IMF variation: the
2019) to define an SFMS and to sample star-forming galaxies in each snapshot
  • Mstar and SFRs of galaxies,
  • 2019
Star formation
εr = 0.2 which is consistent with the value used in the simulations (Churazov et al
  • 2014