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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 2018Show all

9 papers · 1 filter

astro-ph.GA2018★ 193 cited

Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes

Tyrone E. Woods, Bhaskar Agarwal, Volker Bromm +30

In recent years, the discovery of massive quasars at z~7 has provided a striking challenge to our understanding of the origin and growth of supermassive black holes in the early Un…

astro-ph.GA2018★ 55 cited

Production of atomic hydrogen by cosmic rays in dark clouds

Marco Padovani, Daniele Galli, Alexei V. Ivlev +2

The presence of small amounts of atomic hydrogen, detected as absorption dips in the 21 cm line spectrum, is a well-known characteristic of dark clouds. The abundance of hydrogen a…

astro-ph.GA2018★ 54 cited

Witnessing galaxy assembly at the edge of the reionization epoch

V. D'Odorico, C. Feruglio, A. Ferrara +8

We report the discovery of Serenity-18, a galaxy at z=5.939 for which we could measure the content of molecular gas, M(H_2)~ 5 x10^9 M_sun, traced by the CO(6-5) emission, together…

astro-ph.GA2018★ 57 cited

Spectroscopic investigation of a reionized galaxy overdensity at z=7

M. Castellano, L. Pentericci, E. Vanzella +17

We present deep spectroscopic follow-up observations of the Bremer Deep Field (BDF) where the two 7 bright Ly emitters (LAE) BDF521 and BDF3299 were previously discovered…

astro-ph.GA2018★ 5 cited

Growth problems of stellar black holes in early galaxies

Maria Carmela Orofino, Andrea Ferrara, Simona Gallerani

The nature of the seeds of the observed high-z super-massive black holes (SMBH) is unknown. Although different options have been proposed, involving e.g. intermediate mass direct c…

astro-ph.GA2018★ 49 cited

The dense molecular gas in the QSO SDSS J231038.88+185519.7 resolved by ALMA

C. Feruglio, F. Fiore, S. Carniani +13

We present ALMA observations of the CO(6-5) and [CII] emission lines and the sub-millimeter continuum of the quasi-stellar object (QSO) SDSS J231038.88+185519.7. Compared…