미해결 펄서가 초고에너지 은하 확산 감마선 방출에 미치는 영향
초고에너지 은하 확산 감마선 방출에서 미해결 펄서의 기여도는 이전 연구에서 추정했던 것보다 낮으며, 특히 은하계 외곽에서는 미미한 수준이다.
S255IR NIRS3 周囲のジェットと円盤におけるイオン化ガスと分子ガスの微細構造と運動：高解像度ALMA観測からの知見
高解像度ALMA観測により、大質量原始星S255IR NIRS3を取り巻くジェットと円盤の構造が明らかになり、星形成における降着と噴出の複雑なプロセスに関する新たな知見が得られた。
Systematic Identification of Supergiants in M31 and M33 Using LAMOST DR10 Data
This research paper presents a systematic identification of supergiant stars in the nearby galaxies M31 and M33 using spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 10 (DR10).
Detection of Ultrahigh-Energy Gamma Rays from Microquasars: Evidence for Efficient Particle Acceleration in Black Hole-Jet Systems
Observations from the Large High Altitude Air Shower Observatory (LHAASO) reveal ultrahigh-energy gamma-ray emissions from five microquasars, indicating that these black hole-jet systems can accelerate particles to extremely high energies, potentially contributing to Galactic cosmic rays.
Spectral Analysis of A2744-QSO1: Challenges in Modeling the Triply Imaged Little Red Dot
Current AGN and galaxy formation models struggle to explain the unique spectral characteristics of A2744-QSO1, a compact, high-redshift galaxy observed by JWST, suggesting a need for revised understanding of early galaxy evolution.
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