activity
20122022
most citedThe Evolution of Supermassive Population III Stars

168 citations · 774 across the 21 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 18 cited

General-relativistic instability in hylotropic supermassive stars

Lionel Haemmerlé

The formation of supermassive black holes by direct collapse would imply the existence of supermassive stars (SMSs) and their collapse through the general-relativistic (GR) instabi…

astro-ph.HE2020★ 27 cited

Rapidly accreting supermassive stars: reliable determination of the final mass

Lionel Haemmerlé

Supermassive black holes might form by direct collapse, with a supermassive star (SMS) as progenitor. In this scenario, the SMS accretes at > 0.1 Msun/yr until it collapses into a…

astro-ph.SR2020★ 42 cited

On the Origin of the Bimodal Rotational Velocity Distribution in Stellar Clusters: Rotation on the Pre-Main Sequence

Nate Bastian, Sebastian Kamann, Louis Amard +3

We address the origin of the observed bimodal rotational distribution of stars in massive young and intermediate age stellar clusters. This bimodality is seen as split main sequenc…

astro-ph.SR2020★ 53 cited

The IACOB project. VI. On the elusive detection of massive O-type stars close to the ZAMS

G. Holgado, S. Simón-Díaz, L. Haemmerlé +7

The apparent lack of massive O-type stars near the zero-age main sequence (at ages < 2 Myr) is a topic widely discussed. Different explanations for this elusive detection have been…

astro-ph.GA2020★ 32 cited

On Monolithic Supermassive Stars

Tyrone E. Woods, Alexander Heger, Lionel Haemmerlé

Supermassive stars have been proposed as the progenitors of the massive () quasars observed at . Prospects for directly detecting supermassive…

astro-ph.GA2020★ 74 cited

Formation of the first stars and black holes

Lionel Haemmerlé, Lucio Mayer, Ralf S. Klessen +3

We review the current status of knowledge concerning the early phases of star formation during cosmic dawn. This includes the first generations of stars forming in the lowest mass…