activity
20242026
most citedA potential mass-gap black hole in a wide binary with a circular orbit

33 citations · 77 across the 13 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2026★ 1 cited

PhDLspec: physical-prior embedded deep learning method for spectroscopic determination of stellar labels in high-dimensional parameter space

Tianmin Wu, Maosheng Xiang, Jianrong Shi +4

Unlocking the full physical information encoded in low-resolution spectra poses a significant challenge for astronomical survey analysis. Such a task demands modeling spectra and o…

astro-ph.GA2025★ 3 cited

A large, long-lived, slowly-expanding superbubble across the Perseus Arm

Bingqiu Chen, Guangxing Li, Haibo Yuan +5

Stellar feedback is a crucial mechanism in galactic evolution, as demonstrated by the widespread bubbles observed with JWST. In this study, we combine data from Gaia and LAMOST to…

astro-ph.GA2025

Intergalactic Wandering Stars in the Local Universe: Theoretical Predictions for Their Distance and Luminosity Distribution

Jia-Hui Wang, Maosheng Xiang, Ji-Feng Liu

Intergalactic wandering stars (IWSs) within 10 Mpc remain a poorly explored area of astronomy. Such stars, if they exist, are supposed to be wandering objects as they are not bound…

astro-ph.GA2025

Additional Evidence for the Existence of a Primordial Disk System

Shuai Xu, Haibo Yuan, Bowen Huang +7

The origin of very metal-poor (VMP; [Fe/H] ) stars on planar orbits has been the subject of great attention since their first discovery. However, prior to the release of…

astro-ph.GA2024★ 27 cited

The formation and survival of the Milky Way's oldest stellar disk

Maosheng Xiang, Hans-Walter Rix, Hang Yang +3

It remains a mystery when our Milky Way first formed a stellar disk component that survived and maintained its disk structure from subsequent galaxy mergers. We present a study of…

astro-ph.GA2024★ 1 cited

Determining Stellar Elemental Abundances from DESI Spectra with the Data-Driven Payne

Meng Zhang, Maosheng Xiang, Yuan-Sen Ting +8

Stellar abundances for a large number of stars are key information for the study of Galactic formation history. Large spectroscopic surveys such as DESI and LAMOST take median-to-l…