Investigation of projected rotational velocities of Be-type stars in LAMOST DR7

arXiv:2607.15540 · astro-ph.SR · Submitted 2026-07-17 · Read on arXiv

Zhicun Liu, Jiao Li, Jiaming Liu, Xiao-Long Wang, Guozhen Hu, Wenyuan Cui

astro-ph.SR

Submitted: 2026-07-17

Comments: 16 pages, 13 figures, 3 tables

Journal ref: published in ApJ (2026)

DOI: 10.3847/1538-4357/ae7713

Project page: https://archive.stsci.edu/prepds/bosz

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Metallicity — 13× in this paper · explained in 3 episodes
alpha — 3× in this paper · explained in 1 episode
Abundance — 2× in this paper · explained in 1 episode
LAMOST Medium-resolution Survey — 2× in this paper
Milky Way — 2× in this paper
Angular Momentum Loss — 1× in this paper · explained in 1 episode
Core — 1× in this paper · explained in 2 episodes
Large Magellanic Cloud — 1× in this paper
Small Magellanic Cloud — 1× in this paper

Sources

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