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19942023
most citedHerwig 7.0 / Herwig++ 3.0 Release Note

1.2k citations · 13.1k across the 150 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.SR2022★ 14 cited

Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates

Anna J. G. O'Grady, Maria R. Drout, B. M. Gaensler +9

In previous work we identified a population of 38 cool and luminous variable stars in the Magellanic Clouds and examined 11 in detail in order to classify them as either Thorne-Żyt…

astro-ph.GA2022★ 38 cited

The Cosmic Ultraviolet Baryon Survey (CUBS) V: On the Thermodynamic Properties of the Cool Circumgalactic Medium at

Zhijie Qu, Hsiao-Wen Chen, Gwen C. Rudie +11

This paper presents a systematic study of the photoionization and thermodynamic properties of the cool circumgalactic medium (CGM) as traced by rest-frame ultraviolet absorption li…

astro-ph.GA2022★ 24 cited

Empirical constraints on the turbulence in QSO host nebulae from velocity structure function measurements

Mandy C. Chen, Hsiao-Wen Chen, Michael Rauch +9

We present the first empirical constraints on the turbulent velocity field of the diffuse circumgalactic medium around four luminous QSOs at --1.1. Spatially exten…

astro-ph.GA2022★ 104 cited

EMPRESS. V. Metallicity Diagnostics of Galaxies over 12+log(O/H)=~6.9-8.9 Established by a Local Galaxy Census: Preparing for JWST Spectroscopy

Kimihiko Nakajima, Masami Ouchi, Yi Xu +13

We present optical-line gas metallicity diagnostics established by the combination of local SDSS galaxies and the largest compilation of extremely metal-poor galaxies (EMPGs) inclu…

astro-ph.CO2022★ 104 cited

EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension

Akinori Matsumoto, Masami Ouchi, Kimihiko Nakajima +42

The primordial He abundance is a powerful probe of cosmology. Currently, is best determined by observations of metal-poor galaxies, while there are on…