Monthly Notices of the Royal Astronomical Society

First VLBI imaging of SiO v = 0, J = 1→0 masers in VY Canis Majoris

• Abstract

Hubble’s Variable Nebula I: Ripples on a Big Screen

• Abstract
• Supplementary data

Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe

• Abstract

Early evolution of super-Eddington accretion flow in tidal disruption events

• Abstract

ExoMol Photodissociation Cross Sections – II: Continuum Absorption and Predissociation Spectra for the Hydroxyl Radical

• Abstract

FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structure

• Abstract

Can planet–planet binaries survive in star-forming regions?

• Abstract

Searching for star formation towards the Eos molecular cloud

• Abstract

Physical properties and gas kinematics of massive star forming region G328.24−0.55

• Abstract

Broadband study of the SMC pulsar RX J0032.9-7348 during its X-ray brightening in 2024

• Abstract

Modelling JWST mid-infrared counts II: Extension to 5.6 μm, optical, radio and X-rays

• Abstract
• Supplementary data

A Neural Network Model for the Cosmic Dispersion Measure in the CAMELS Simulations

• Abstract

Exogenic dust inventory in the Saturn system: the Cassini Cosmic Dust Analyzer perspective

• Abstract

Geometric Mean Algebraic Reconstruction Technique : A tool for ionospheric tomography using GNSS receiver system

• Abstract

DESI Peculiar Velocity Survey – Fundamental Plane

• Abstract

Mapping the cosmic gamma-ray horizon: the 1CGH catalogue of Fermi-LAT detections above 10 GeV

• Abstract
• Supplementary data

AT 2018dyk: tidal disruption event or active galactic nucleus? Follow-up observations of an extreme coronal line emitter with the Dark Energy Spectroscopic Instrument

• Abstract

Modeling Rotational State Changes in C₃N⁻ and CN⁻ by Collision with H in Interstellar Environments

• Abstract
• Supplementary data

Estimating constraints on cosmological parameters via the canonical and the differential redshift drift with SKA HI 21-cm observations

• Abstract