Siming Liu, Ph.D.
Affiliations: | 2002 | University of Arizona, Tucson, AZ |
Area:
Astronomy and AstrophysicsGoogle:
"Siming Liu"Mean distance: 4517.33
Parents
Sign in to add mentor| Fulvio Melia | grad student | 2002 | University of Arizona | |
| (Accretion processes around supermassive black holes.) | ||||
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Publications
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| Liu S, Zeng H, Xin Y, et al. (2020) Hadronic versus Leptonic Models for γ-Ray Emission from VER J2227+608 The Astrophysical Journal. 897 |
| Zhou X, Muñoz PA, Büchner J, et al. (2020) Wave excitation by energetic ring-distributed electron beams in the solar corona The Astrophysical Journal. 891: 92 |
| Zhang H, Xi S, Liu R, et al. (2020) Discovery of a Spatially Extended GeV Source in the Vicinity of the TeV Halo Candidate 2HWC J1912+099: a TeV Halo or Supernova Remnant? The Astrophysical Journal. 889: 12 |
| Xin Y, Zeng H, Liu S, et al. (2019) VER J2227+608: A Hadronic PeVatron Pulsar Wind Nebula? The Astrophysical Journal. 885: 162 |
| Bao Y, Liu S, Chen Y. (2019) On the Gamma-Ray Nebula of Vela Pulsar. I. Very Slow Diffusion of Energetic Electrons within the TeV Nebula The Astrophysical Journal. 877: 54 |
| Zhang X, Liu S. (2019) Electron Acceleration in Middle-age Shell-type γ-Ray Supernova Remnants The Astrophysical Journal. 876: 24 |
| Zhu Z, Li Z, Morris MR, et al. (2019) A Deep Chandra View of a Candidate Parsec-scale Jet from the Galactic Center Supermassive Black Hole The Astrophysical Journal. 875: 44 |
| Zhang X, Liu S. (2019) Is Supernova Remnant Cassiopeia A a PeVatron The Astrophysical Journal. 874: 98 |
| Zeng H, Xin Y, Liu S. (2019) Evolution of High-energy Particle Distribution in Supernova Remnants The Astrophysical Journal. 874: 50 |
| Shi Z, Liu S. (2019) Origin of Cosmic Ray Electrons and Positrons Monthly Notices of the Royal Astronomical Society. 485: 3869-3875 |