New preprints from Astrophysics Letters describe work in progress on Work Package 4.5 for the Wide-field Spectroscopic Telescope (WST), a planned 12-meter-class facility focused on large spectroscopic surveys. The Wide-field Spectroscopic Telescope High-Resolution Multi-Object Spectrograph (MOS-HR / HR-MOS) is designed to deliver a resolving power of R = 40,000 and a multiplexing capability of about 2,000 targets. One paper details the mechanical design and optomechanical architecture for the high-resolution spectrograph. It presents an approach that divides the instrument into four larger modules, each made up of two sub-modules, using a vertical optical bench configuration with optical elements mounted on both sides. The authors describe steps for translating the baseline optical prescription into a full mechanical model, defining mounting and alignment interfaces, and conducting preliminary static, modal, and seismic analyses to assess performance under operational and survival loads. Another paper reports the current status of the HR-MOS, including the organization of an international team and how the optical design has evolved through trade-off studies driven by scientific requirements and technical constraints, as well as envelope dimensions and mass estimates, fiber specifications, and structural stability analyses. Both reports describe modular architecture and include mechanical performance evaluations alongside feasibility considerations.