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20002026
most citedCold gas accretion in galaxies

598 citations · 8.2k across the 149 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.GA2019★ 18 cited

Introduction to Galaxy Formation and Evolution. From Primordial Gas to Present-Day Galaxies

Andrea Cimatti, Filippo Fraternali, Carlo Nipoti

Present-day elliptical, spiral and irregular galaxies are large systems made of stars, gas and dark matter. Their properties result from a variety of physical processes that have o…

astro-ph.GA2019★ 40 cited

The volumetric star formation law in the Milky Way

C. Bacchini, F. Fraternali, G. Pezzulli +3

Several open questions on galaxy formation and evolution have their roots in the lack of a universal star formation law, that could univocally link the gas properties, e.g. its den…

astro-ph.GA2019

Baryon dominated ultra-diffuse galaxies

Pavel E. Mancera Piña, Filippo Fraternali, Elizabeth A. K. Adams +1

By means of interferometic 21-cm observations and a 3D kinematic modeling technique, we study the gas kinematics of six HI-rich ultra-diffuse galaxies (UDGs). We derive robust circ…

astro-ph.GA2019★ 65 cited

HALOGAS: the properties of extraplanar HI in disc galaxies

A. Marasco, F. Fraternali, G. Heald +9

We present a systematic study of the extraplanar gas (EPG) in a sample of 15 nearby late-type galaxies at intermediate inclinations using publicly available, deep interferometric H…

astro-ph.GA2019★ 149 cited

Off the baryonic Tully-Fisher relation: a population of baryon-dominated ultra-diffuse galaxies

Pavel E. Mancera Piña, Filippo Fraternali, Elizabeth A. K. Adams +17

We study the gas kinematics traced by the 21-cm emission of a sample of six HIrich low surface brightness galaxies classified as ultra-diffuse galaxies (UDGs). Using the 3D kine…

astro-ph.GA2019★ 50 cited

Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching

Lorenzo Posti, Antonino Marasco, Filippo Fraternali +1

In CDM cosmology, to first order, galaxies form out of the cooling of baryons within the virial radius of their dark matter halo. The fractions of mass and angular momentum reta…