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20102025
most citedRed Supergiant Stars in the Large Magellanic Cloud: I. The Period-Luminosity Relation

59 citations · 487 across the 30 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 14 cited

Dust Extinction Law in Nearby Star-Resolved Galaxies. I. M31 Traced by Supergiants

Yuxi Wang, Jian Gao, Yi Ren

The dust extinction laws and dust properties in M31 are explored with a sample of reddened O-type and B-type supergiants obtained from the LGGS. The observed spectral energy distri…

astro-ph.GA2021★ 3 cited

The Dust Mass of Supernova Remnants in M31

Ye Wang, Biwei Jiang, Jun Li +2

The dust temperature and mass of the supernova remnants (SNRs) in M31 are estimated by fitting the infrared spectral energy distribution calculated from the images in the Spitzer/I…

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.GA2021★ 19 cited

The Extinction and Distance of the MBM Molecular Clouds at High Galactic Latitude

Mingxu Sun, Biwei Jiang, He Zhao +1

Based on the accurate color excess of more than 4 million stars and of more than 1 million stars from \citet{2021ApJS..254...38S}, the…

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.SR2021★ 16 cited

Evolved Massive Stars at Low-metallicity IV. Using 1.6 m "H-bump" to identify red supergiant stars: a case study of NGC 6822

Ming Yang, Alceste Z. Bonanos, Biwei Jiang +9

We present a case study of using a novel method to identify red supergiant (RSG) candidates in NGC 6822, based on their 1.6 m "H-bump". We collected 32 bands of photometric data…