activity
20172022
most citedStar formation in a galactic outflow

240 citations · 617 across the 9 of their papers we have counts for

collaborators

14 papers

astro-ph.GA202266 cited

Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts

Alice Concas, Roberto Maiolino, Mirko Curti +13

We investigate the presence of ionised gas outflows in a sample of 141 main-sequence star-forming galaxies at from the KLEVER (KMOS Lensed Emission Lines and VElocity R…

astro-ph.GA202210 cited

Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models

Jingjing Shi, Yingjie Peng, Benedikt Diemer +15

Black hole feedback has been widely implemented as the key recipe to quench star formation in massive galaxies in modern semi-analytic models and hydrodynamical simulations. As the…

astro-ph.GA202135 cited

SUPER. VI. A giant molecular halo around a z~2 quasar

C. Cicone, V. Mainieri, C. Circosta +16

We present the discovery of copious molecular gas in the halo of cid_346, a quasar studied as part of the SINFONI survey for Unveiling the Physics and Effect of Radiative f…

astro-ph.GA202135 cited

The diffuse ionized gas (DIG) in star-forming galaxies: the influence of aperture effects on local HII regions

F. Mannucci, F. Belfiore, M. Curti +7

The Diffuse Ionized Gas (DIG) contributes to the nebular emission of galaxies, resulting in emission line flux ratios that can be significantly different from those produced by HII…

astro-ph.GA2021

From haloes to galaxies. III. The gas cycle of local galaxy populations

Jing Dou, Yingjie Peng, Alvio Renzini +12

In Dou et al. (2021), we introduced the Fundamental Formation Relation (FFR), a tight relation between specific SFR (sSFR), H star formation efficiency (SFE), and t…

astro-ph.GA202117 cited

Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe

Chengpeng Zhang, Yingjie Peng, Luis C. Ho +13

The phenomenological study of evolving galaxy populations has shown that star forming galaxies can be quenched by two distinct processes: mass quenching and environment quenching (…