RNA-seq
Emission Spectra
Multi-species Conserved Sequences
Atomic Emission Spectroscopy: Overview
Additional Subnuclear Structures
Additional Subnuclear Structures
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Updated: Jan 7, 2026

3' End Sequencing Library Preparation with A-seq2
Published on: October 10, 2017
Chengyuan Li1,2, Antonino P Milone3,4, Weijia Sun5
1School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519082, China.
Extended main sequences and turn-offs challenge simple stellar population models. Stellar rotation is the most likely cause, offering new insights into stellar astrophysics and cluster evolution.
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