activity
20202024
most citedEvolved Massive Stars at Low-metallicity V. Mass-Loss Rate of Red Supergiant Stars in the Small Magellanic Cloud

59 citations · 160 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2024

Evolved Massive Stars at Low-metallicity VI. Mass-Loss Rate of Red Supergiant Stars in the Large Magellanic Cloud

Jing Wen, Jian Gao, Ming Yang +4

Mass loss is a crucial process that affects the observational properties, evolution path and fate of highly evolved stars. However, the mechanism of mass loss is still unclear, and…

astro-ph.SR2023★ 59 cited

Evolved Massive Stars at Low-metallicity V. Mass-Loss Rate of Red Supergiant Stars in the Small Magellanic Cloud

Ming Yang, Alceste Z. Bonanos, Biwei Jiang +17

We assemble the most complete and clean red supergiant (RSG) sample (2,121 targets) so far in the Small Magellanic Cloud (SMC) with 53 different bands of data to study the MLR of R…

astro-ph.SR2022★ 5 cited

Infrared Excess of a Large OB Star Sample

Dingshan Deng, Yang Sun, Tianding Wang +2

The infrared excess from OB stars are commonly considered as contributions from ionized stellar wind or circumstellar dust. With the newly published LAMOST-OB catalog and GOSSS dat…

astro-ph.GA2021★ 32 cited

The Sample of Red Supergiants in Twelve Low-Mass Galaxies of the Local Group

Yi Ren, Biwei Jiang, Ming Yang +2

This work establishes the most complete sample of red supergiants (RSGs) in twelve low-mass galaxies (WLM, IC 10, NGC 147, NGC 185, IC 1613, Leo A, Sextans B, Sextans A, NGC 6822,…

astro-ph.SR2021★ 28 cited

Red supergiants in M31 and M33 II. The Mass Loss Rate

Tianding Wang, Biwei Jiang, Yi Ren +2

Mass loss is an important activity for red supergiants (RSGs) which can influence their evolution and final fate. Previous estimations of mass loss rates (MLRs) of RSGs exhibit sig…

astro-ph.SR2020★ 36 cited

Red Supergiants in M31 and M33 I. The Complete Sample

Yi Ren, Biwei Jiang, Ming Yang +3

The aim of this paper is to establish a complete sample of red supergiants (RSGs) in M31 and M33. The member stars of the two galaxies are selected from the near-infrared (NIR) poi…