activity
20102026
most citedThe Hamburg/ESO R-process Enhanced Star survey (HERES) VI. The Galactic Chemical Evolution of Silicon

23 citations · 60 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Carbon in J0815+4729: Casting a shadow of doubt on the interpretation of CH absorption in the most primitive stars

Junbo Zhang, Carlos Allende Prieto, Yeisson Osorio +7

Aims. We revisit the carbon abundance in the primitive iron-poor star J0815+4729 ([Fe/H] = -5.49). J0815+4729 is so carbon-enhanced and oxygen-rich that, in addition to CH and C2 m…

astro-ph.GA2025★ 1 cited

Milky Way Mass Through Escape Velocity Curve from LAMOST K Giants

Yin Wu, Haining Li, Yang Huang +2

Escape velocity has long been used to constrain the mass of the Dark Matter (DM) halo in the Milky Way (MW). Here we present a study of the escape velocity curve using a sample of…

astro-ph.GA2025★ 2 cited

Unveiling Galactic substructures with M Giant stars: A kinematic and chemical study based on LAMOST DR9, Gaia DR3 and APOGEE DR17

Longfei Ding, Jing Li, Xiang-Xiang Xue +3

Based on the updated M giant star catalog selected from LAMOST DR9, we iden-tify substructures within the integrals-of-motion space through Friends-of-Friends cluster-ing algorithm…

astro-ph.SR2025★ 5 cited

An Actinide-boost Star Discovered in the Gaia-Sausage-Enceladus

Yangming Lin, Haining Li, Ruizheng Jiang +6

We report the discovery of an actinide-boost, very metal-poor (), -process-enhanced () star, LAMOST J0804+5…

astro-ph.SR2025★ 3 cited

The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars

Xizhen Lu, Chunhua Zhu, Guoliang Lü +3

The detection of the neutrino magnetic moment (NMM,) is one of the most significant challenges in physics. The additional energy loss due to NMM can significantly influence th…

astro-ph.SR2024

Study of a red clump giant, KIC~11087027, with high rotation and strong infrared excess -- Evidence of tidal interaction for high lithium abundance

Raghubar Singh, Anohita Mallick, Bacham E. Reddy +2

This paper presents results from Kepler photometric light curves and high-resolution spectroscopic study of a super Li-rich giant KIC11087027. Using the light curve analysis, we me…

astro-ph.GA2024★ 19 cited

Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties

Ruizhi Zhang, Tadafumi Matsuno, Haining Li +9

Very metal-poor (VMP) stars record the signatures of early accreted galaxies, making them essential tools for unraveling the early stages of Galaxy formation. Understanding the ori…

astro-ph.GA2024★ 5 cited

Detection of the actinide Th in an r-process-enhanced star with accretion origin

Xing Qianfan, Zhao Gang, Aoki Wako +4

The thorium and six second-peak r-process element (56<Z<72) abundances are determined for the alpha-poor star LAMOST J1124+4535 based on a high-resolution spectrum obtained with th…

astro-ph.GA2024★ 2 cited

Kinematical Fluctuations Vary with Galaxy Surface Mass Density

Ze-Hao Zhong, Gang Zhao, Hans-Walter Rix +1

The Galaxy inner parts are generally considered to be optically symmetric, as well as kinematically symmetric for most massive early-type galaxies. At the lower-mass end, many gala…

astro-ph.SR2023

Unique chemical composition of the very metal-poor star LAMOST J1645+4357

Wako Aoki, Haining Li, Nozomu Tominaga +3

We report on the chemical composition of the very metal-poor ([Fe/H]=-2.9) star LAMOST J1645+4357 that is identified to be a red giant having peculiar abundance ratios by Li et al.…

astro-ph.SR2010★ 23 cited

The Hamburg/ESO R-process Enhanced Star survey (HERES) VI. The Galactic Chemical Evolution of Silicon

L. Zhang, T. Karlsson, N. Christlieb +3

We determined the silicon abundances of 253 metal-poor stars in the metallicity range , based on non-local thermodynamic equilibrium (NLTE) line formation…