Conveners
Plenary talks
- Yuhui DONG Yuhui (BSRF, IHEP, CAS)
Plenary talks: Plenary and SNR
- Yang Chen (Nanjing University)
Up to now, the LHAASO collaboration have signed ten Memorandum of Understandings (MoUs), including seven international ones and three domestic ones, with the other collaborations on joint analysis. The facilities of The joint collaborations include ground radio, gamma ray, neutrino telescopes and observatories on satelites, so that the joint field covers multi-waveband astronomy and...
Based on the results of SNR G150.3+4.5 at the 38th International Cosmic Ray Conference (ICRC2023), we updated several main results: (1) Using the updated data, we obtained two Gaussian distributions, which basically corresponded to the energy segments of WCDA and KM2A by conjoint analyzing WCDA and KM2A data; (2) Using CO data from the Milky Way Imaging Scroll Painting survey (MWISP), it is...
It is difficult to identify hadronic PeVatrons (the PeV particle accelerator) from the ultra-high-energy (UHE, E>100TeV) gamma-ray sources, which is however crucial in revealing the origin of cosmic rays. As an endeavor in this regard, we focus in this work on the UHE gamma-ray source 1LHAASO J1857+0203u, which may associate with the supernova remnant (SNR) G35.6−0.4 and H II region G35.6−0.5....
Identification of cosmic-ray (CR) accelerators, especially those that can accelerate protons up to PeV regime (namely, PeVatrons), is one of major goals of high-energy astrophysics and plays a crucial role in understanding the origin of Galactic CRs. In this contribution, we report the LHAASO obsesrvation on an intriguing SNR-PWN complex consisting of the famous PeVatron candidate SNR...
