1.7k citations
- Chinese Academy of SciencesCN538 papers
- University of Chinese Academy of SciencesCN288 papers
- National Astronomical ObservatoriesCN203 papers
- Peking UniversityCN69 papers
- University of Science and Technology of ChinaCN59 papers
- Nanjing UniversityCN58 papers
- Shanghai Astronomical ObservatoryCN58 papers
- Kavli Institute for Theoretical SciencesCN56 papers
- Centre National de la Recherche ScientifiqueFR48 papers
- Korea Astronomy and Space Science InstituteKR45 papers
- Purple Mountain ObservatoryCN45 papers
- Tsinghua UniversityCN41 papers
74 papers · 1 filter
How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
Yongda Zhu, Hai-Xia Ma, Xiao-Bo Dong +7
Aiming at discriminating different gravitational potential models of the Milky Way, we perform tests based on the kinematic data powered by the Gaia DR2 astrometry, over a large ra…
Modelling the magnetic structure of a large-scale horse-shoe-like filament in a decaying and diffuse active region
Kaifeng Kang, Yang Guo, Ilia I. Roussev +2
A large-scale, horse-shoe-like filament was investigated and the magnetic field around it was reconstructed. This is an intermediate filament (IF) that appeared on the solar disk f…
Detecting the oscillation and propagation of the nascent dynamic solar wind structure at 2.6 solar radii using VLBI radio telescopes
Maoli Ma, Guifre Molera Calves, Giuseppe Cimo +29
Probing the solar corona is crucial to study the coronal heating and solar wind acceleration. However, the transient and inhomogeneous solar wind flows carry large-amplitude inhere…
Hydrodynamical simulations for the common-envelope wind model for Type Ia supernovae
Yingzhen Cui, Xiangcun Meng, Philipp Podsiadlowski +1
The single-degenerate (SD) model is one of the leading models for the progenitors of Type Ia supernovae (SNe Ia). Recently, a new version of the SD model, the common-envelope wind…
Dynamical masses of the primary Be star and the secondary sdB star in the single-lined binary kappa Dra (B6 IIIe)
R. Klement, D. Baade, Th. Rivinius +16
Because many classical Be stars may owe their nature to mass and angular-momentum transfer in a close binary, the present masses, temperatures, and radii of their components are of…
An 18.9-minute Blue Large-Amplitude Pulsator Crossing the 'Hertzsprung Gap' of Hot Subdwarfs
Jie Lin, Chengyuan Wu, Xiaofeng Wang +28
Blue large-amplitude pulsators (BLAPs) represent a new and rare class of hot pulsating stars with unusually large amplitudes and short periods. Up to now, only 24 confirmed BLAPs h…