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20102026
most citedRed Supergiant Stars in the Large Magellanic Cloud: I. The Period-Luminosity Relation

59 citations · 86 across the 5 of their papers we have counts for

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astro-ph.SR2026

JWST Reveals a Galaxy-Wide Association of Red Supergiants with OB Stars in NGC 5584

Min Dai, Shu Wang, Biwei Jiang

The spatial relationship between young and evolved massive-star tracers offers a means of probing recent star formation across galactic disks. We combine JWST/NIRCam, /UVOT…

astro-ph.SR2025

The Samples and Binary Fractions of Red Supergiant in M31 and M33 by the HST Observations

Min Dai, Shu Wang, Biwei Jiang +1

The binarity of red supergiants (RSGs) influences their evolution and the fate of supernovae. We investigate the binary fraction of RSGs in the Andromeda Galaxy (M31) and Triangulu…

astro-ph.SR2025

The Binary Fraction of Red Supergiants in the Magellanic Clouds

Min Dai, Shu Wang, Biwei Jiang

Red supergiants (RSGs), as the descendants of OB-type stars and the progenitors of supernovae, provide crucial insights into the evolution of massive stars, particularly in binary…

astro-ph.SR2024

Evolved Massive Stars at Low-metallicity VII. the Lower Mass Limit of Red Supergiant Population in the Large Magellanic Cloud

Ming Yang, Bo Zhang, Biwei Jiang +8

The precise definition of the lower mass limit of red supergiant stars (RSGs) is an open question in astrophysics and does not attract too much attention. Here we assemble a spectr…

astro-ph.SR2020★ 27 cited

Evolved Massive Stars at Low-metallicity II. Red Supergiant Stars in the Small Magellanic Cloud

Ming Yang, Alceste Z. Bonanos, Bi-Wei Jiang +9

We present the most comprehensive RSG sample for the SMC up to now, including 1,239 RSG candidates. The initial sample is derived based on a source catalog for the SMC with conserv…

astro-ph.SR2018

Red supergiant stars in the Large Magellanic Cloud. II. Infrared properties and mid-infrared variability

Ming Yang, Alceste Z. Bonanos, Bi-Wei Jiang +7

The characteristics of IR properties and MIR variability of RSGs in the LMC are analyzed based on 12 bands of NIR to MIR co-added data from 2MASS, Spitzer and WISE, and 6.6 y…