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20152024
most citedConstraining mixing in massive stars in the Small Magellanic Cloud

130 citations · 823 across the 26 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.HE2021★ 19 cited

Explodability fluctuations of massive stellar cores enable asymmetric compact object mergers such as GW190814

John Antoniadis, David R. Aguilera-Dena, Alejandro Vigna-Gómez +6

The first three observing runs with Advanced LIGO and Virgo have resulted in the detection of binary black hole mergers (BBH) with highly unequal mass components, which are difficu…

astro-ph.GA2021★ 13 cited

A wide-field CO survey towards the California Molecular Filament

Weihua Guo, Xuepeng Chen, Jiancheng Feng +9

We present the survey of CO/CO/CO (J=1-0) toward the California Molecular Cloud (CMC) within the region of 161.75 167.75$^{\cir…

astro-ph.GA2021★ 13 cited

Improved Measurements of Molecular Cloud Distances Based on Global Search

Qing-Zeng Yan, Ji Yang, Yang Su +5

The principle of the background-eliminated extinction-parallax (BEEP) method is examining the extinction difference between on- and off-cloud regions to reveal the extinction jump…

astro-ph.SR2021★ 55 cited

The young massive SMC cluster NGC 330 seen by MUSE II. Multiplicity properties of the massive-star population

J. Bodensteiner, H. Sana, C. Wang +10

Observations of massive stars in young open clusters (< ~8 Myr) have shown that a majority of them are in binary systems, most of which will interact during their life. Populations…

astro-ph.GA2021★ 14 cited

On the Beam Filling Factors of Molecular Clouds

Qing-Zeng Yan, Ji Yang, Yang Su +2

Imaging surveys of CO and other molecular transition lines are fundamental to measuring the large-scale distribution of molecular gas in the Milky Way. Due to finite angular resolu…

astro-ph.GA2021★ 29 cited

Molecular gas distribution perpendicular to the Galactic plane

Yang Su, Ji Yang, Qing-Zeng Yan +9

We use the ~370 square degrees data from the MWISP CO survey to study the vertical distribution of the molecular clouds (MCs) toward the tangent points in the region of l=[16,52]de…