2022年3期
Research in Astronomy and Astrophysics
- The Precision Analysis of the Chinese VLBI Network in Probe Delay Measurement
- The Origin of The Soft X-Ray Excess in the Seyfert 1.5 Galaxy ESO 362-G18
- FAST Continuum Mapping of the SNR VRO 42.05.01
- Fast Radio Bursts as Crustal Dynamical Events Induced by Magnetic Field Evolution in Young Magnetars
- Is TOL 1326–379 a Prototype of γ-Ray Emitting FR0 Radio Galaxy?
- Precise Positions of Triton in 2010–2014 based on Gaia-DR2
- Spatial Distribution of HOCN Around Sagittarius B2
- Evaluating Helium Variations By Modeling Red Giant Branch Bump of Large Magellanic Cluster NGC 1978
- The First Photometric Analysis of Two Low Mass Ratio Totally Eclipsing Contact Binaries:TIC 393943031 and TIC 89428764
- Application of a Space-based Optical Interferometer Toward Measuring Cosmological Distances of Quasars
- Method of Separating Cosmic-Ray Positrons from Electrons in the DAMPE Experiment
- The New Wuqing 70m Radio Telescope and Measurements of Main Electronic Properties in the X-band
- Optical Properties of C-rich (12C,SiC and FeC) Dust Layered Structure of Massive Stars*
- Temperature Analysis of Flaring (AR 11283) and Non-flaring (AR 12194)Coronal Loops
- Transonic Accretion and Winds Around Pseudo-Kerr Black Holes And Comparison with General Relativistic Solutions
- Radiative Diffusion in a Time-dependent Outflow:a Model for Fast Blue Optical Transients
- Analysis of the Distribution,Rotation and Scale Characteristics of Solar Wind Switchbacks:Comparison between the First and Second Encounters of Parker Solar Probe
- Imprints of the Jittering Jets Explosion Mechanism in the Morphology of the Supernova Remnant SNR 0540-69.3
- Solving Surface Deformation of Radio Telescope Antenna by Artificial Neural Network
- New Massive Contact Twin Binary in a Radio-quiet HII Region Associated with the M17 Complex
- Physical Properties of 29 sdB+dM Eclipsing Binaries in Zwicky Transient Facility
- Hypercritical Accretion for Black Hole High Spin in Cygnus X-1
- V0644 Ser:An Active Ultrashort Period Contact Binary Star
- Common Envelope to Explosion Delay time Distribution (CEEDTD) of Type Ia Supernovae
- Influence of Megaregolith on the Thermal Evolution of Mercury’s SilicateShell
- Estimation of HII Bubble Size Distribution from 21cm Power Spectrum with Artificial Neural Networks