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19932026
most citedStarburst-driven Mass Loss from Dwarf Galaxies: Efficiency and Metal Ejection

991 citations · 18.7k across the 255 of their papers we have counts for

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Showing 2019Show all

15 papers · 1 filter

astro-ph.GA2019★ 36 cited

Supernovae within Pre-existing Wind-Blown Bubbles: Dust Injection vs. Ambient Dust Destruction

Sergio Martínez-González, Richard Wünsch, Sergiy Silich +3

By means of 3-D hydrodynamical simulations, here we evaluate the impact that supernova explosions occurring within wind-driven bubbles have on the survival or destruction of dust g…

astro-ph.GA2019★ 34 cited

Studying high-z galaxies with [CII] intensity mapping

Bin Yue, Andrea Ferrara

We investigate the [CII] line intensity mapping (IM) signal from galaxies in the Epoch of Reionization (EoR) to assess its detectability, the possibility to constrain the $L_{\rm C…

astro-ph.GA2019★ 16 cited

The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties

V. Allevato, A. Viitanen, A. Finoguenov +10

Aims. We perform clustering measurements of 800 X-ray selected Chandra COSMOS Legacy (CCL) Type 2 AGN with known spectroscopic redshift to probe the halo mass dependence on AGN hos…

astro-ph.GA2019★ 188 cited

Large Population of ALMA Galaxies at z>6 with Very High [OIII]88um to [CII]158um Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

Yuichi Harikane, Masami Ouchi, Akio K. Inoue +20

We present our new ALMA observations targeting [OIII]88um, [CII]158um, [NII]122um, and dust continuum emission for three Lyman break galaxies at z=6.0293-6.2037 identified in the S…

astro-ph.GA2019★ 109 cited

A physical model for [CII] line emission from galaxies

A. Ferrara, L. Vallini, A. Pallottini +5

A tight relation between the [CII]158m line luminosity and star formation rate is measured in local galaxies. At high redshift (), though, a much larger scatter is observed…

astro-ph.GA2019★ 6 cited

Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization

T. K. Daisy Leung, Andrea Pallottini, Andrea Ferrara +1

We study the properties of molecular-forming gas clumps (MGCs) at the epoch of reionization using cosmological zoom-in simulations. We identify MGCs in a z=6 prototypical galaxy ("…