期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (3)
The clustering signals of galaxy clusters are powerful tools for self-calibrating the mass-observable relation and are complementary to cluster abunda......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (3)
Strangeon star model has passed various observational tests, such as the massive pulsars and the tidal deformability during binary mergers. Pulsar gli......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (3)
Recent observations of GN-z11 with JWST/NIRSpec revealed numerous oxygen, carbon, nitrogen, and helium emission lines at z = 10.6. Using the measured ......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (4)
Radio-mode feedback is a key ingredient in galaxy formation and evolution models, required to reproduce the observed properties of massive galaxies in......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (4)
We have studied the pulse-to-pulse variability in PSR J1820-0427 and its frequency dependence using high-quality, wide-band observations made with the......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (4)
Mergers of galaxy clusters are promising probes of dark matter (DM) physics. For example, an offset between the DM component and the galaxy distributi......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (4)
We develop a comprehensive theoretical model for Lyman-alpha (Ly & alpha;) emission, from the scale of individual Ly & alpha; emitters (LAEs) ......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 523 (1)
Quasiperiodic eruptions (QPEs) from low-mass galaxy centres may result from accretion from a white dwarf in a very eccentric orbit about the central m......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (1)
The ionizing radiation of young and massive stars is a crucial form of stellar feedback. Most ionizing (Lyman-continuum; LyC, lambda< 912A) photons......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (1)
Sub-Neptune exoplanets are commonly hypothesized to consist of a silicate-rich magma ocean topped by a hydrogen-rich atmosphere. Previous work studyin......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (2)
We explore constraints on the Milky Way dark matter halo oblateness using three stellar streams from globular clusters NGC3201, M68, and Palomar 5. Pr......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (2)
A recent letter studied cratering during collisions between rocky bodies and primordial black holes. Hydrodynamic simulations in that work showed that......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (2)
If the gravitational lens is surrounded by non-homogeneous plasma, in addition to the vacuum gravitational deflection, chromatic refraction occurs. Al......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (3)
The fast growth of supermassive black holes and their feedback to the host galaxies play an important role in regulating the evolution of galaxies, es......
期刊： MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023; 524 (3)
Radio interferometry calibration and radio frequency interference (RFI) removal are usually done separately. Here we show that jointly modelling the a......
