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Volume 538, Issue 3, April 2025
Articles
Non-LTE radiative transfer simulations: improved agreement of the double detonation with normal Type Ia supernovae
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1289–1300, https://doi.org/10.1093/mnras/staf261
Global 21 cm signal recovery under changing environmental conditions
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1301–1313, https://doi.org/10.1093/mnras/staf315
The arc-shaped radio source at the centre of NGC 6334A: is it a colliding wind region of two young massive stars or the bow shock of a runaway star?
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1314–1328, https://doi.org/10.1093/mnras/staf344
Activity of comet 7P/Pons–Winnecke during the 2021 apparition
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1329–1338, https://doi.org/10.1093/mnras/staf370
Tracing chemical depletion in evolved binaries hosting second-generation transition discs
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1339–1366, https://doi.org/10.1093/mnras/staf375
A census of OB stars within 1 kpc and the star formation and core collapse supernova rates of the Milky Way
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1367–1383, https://doi.org/10.1093/mnras/staf083
3D hydrodynamic simulations of white dwarf-main-sequence star collisions – II. Off-centre collisions
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1384–1396, https://doi.org/10.1093/mnras/staf328
Finding radio transients with anomaly detection and active learning based on volunteer classifications
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1397–1414, https://doi.org/10.1093/mnras/staf336
A field-level emulator for modelling baryonic effects across hydrodynamic simulations
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1415–1426, https://doi.org/10.1093/mnras/staf355
Study on the physical parameters of 18 contact binary stars
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1427–1441, https://doi.org/10.1093/mnras/staf356
emPDF: inferring the Milky Way mass with data-driven distribution function in phase space
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1442–1460, https://doi.org/10.1093/mnras/staf358
Hybrid radiation hydrodynamics scheme with adaptive gravity-tree-based pseudo-particles
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1461–1480, https://doi.org/10.1093/mnras/staf366
FAUST–XXII. Deuteration in the VLA1623-2417 protostellar hot-corinos, cavities, and streamers
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1481–1500, https://doi.org/10.1093/mnras/staf367
Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z = 2.09: implications for black hole–galaxy coevolution and AGN quenching at high redshift
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1501–1516, https://doi.org/10.1093/mnras/staf372
Modelling the Galactic Chemical Evolution of Helium
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1517–1534, https://doi.org/10.1093/mnras/staf373
Evidence of pure ammonia clouds in Jupiter’s Northern Temperate domain from Juno/JIRAM infrared spectral data
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1535–1564, https://doi.org/10.1093/mnras/staf381
Hydrogenation of HOCO and formation of interstellar CO2: a not so straightforward relation
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1565–1575, https://doi.org/10.1093/mnras/staf383
Evidence for relativistic Sunyaev–Zeldovich effect in Planck CMB maps with an average electron-gas temperature of Te ≃ 5 keV
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1576–1586, https://doi.org/10.1093/mnras/staf384
Bar formation and evolution in the cosmological context: inputs from the Auriga simulations
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1587–1608, https://doi.org/10.1093/mnras/staf389
Photometric study of eight distant comets
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1609–1627, https://doi.org/10.1093/mnras/staf400
Unveiling the bulge–disc structure, AGN feedback, and baryon landscape in a massive spiral galaxy with Mpc-scale radio jets
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1628–1652, https://doi.org/10.1093/mnras/staf229
Prospects for biological evolution on Hycean worlds
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1653–1662, https://doi.org/10.1093/mnras/staf094
Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1663–1689, https://doi.org/10.1093/mnras/staf287
CHEXANET: a novel approach to fast-tracking disequilibrium chemistry calculations for exoplanets using neural networks
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1690–1719, https://doi.org/10.1093/mnras/staf297
Asteroseismic study of subgiants and giants of the open cluster M67 using Kepler/K2: expanded sample and precise masses
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1720–1746, https://doi.org/10.1093/mnras/staf353
Investigating pulsating variables and eclipsing binaries in NGC 2126 using ground- and space-based photometry, astrometry, spectroscopy, and modelling
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1747–1772, https://doi.org/10.1093/mnras/staf361
Dynamical heating of newborn stars driven by accretion-induced orbital tightening
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1773–1783, https://doi.org/10.1093/mnras/staf378
VLBA detections in the Oph-S1 binary system near periastron confirmation of its orbital elements and mass
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1784–1788, https://doi.org/10.1093/mnras/staf396
Neural network-based model of galaxy power spectrum: fast full-shape galaxy power spectrum analysis
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1789–1799, https://doi.org/10.1093/mnras/staf285
Contemporaneous optical-radio observations of a fast radio burst in a close galaxy pair
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1800–1815, https://doi.org/10.1093/mnras/staf289
Extraction of H i gas with bulk motions in the disc of galaxies
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1816–1829, https://doi.org/10.1093/mnras/staf298
Fuzzy dark matter constraints from the Hubble Frontier Fields
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1830–1842, https://doi.org/10.1093/mnras/staf340
Scaling relations in the phase-space structure of dark matter haloes
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1843–1852, https://doi.org/10.1093/mnras/staf447
Constraining the scattered light properties of LTT 9779 b using HST/WFC3 UVIS
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1853–1862, https://doi.org/10.1093/mnras/staf402
Correction
Correction to: Can early dark energy be probed by the high-redshift galaxy abundance?
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Page 1863, https://doi.org/10.1093/mnras/staf404
Articles
De-excitation rate coefficients computation of the newly observed thiofulminic acid (HCNS) by collision with helium atoms
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1864–1870, https://doi.org/10.1093/mnras/staf406
Modelling the cool gas clumps in the circumgalactic medium
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1871–1883, https://doi.org/10.1093/mnras/staf407
Nebular emission from composite star-forming galaxies – I. A novel modelling approach
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1884–1905, https://doi.org/10.1093/mnras/staf143
Infrared spectroscopy of astrophysical ice analogues at oblique angles
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1906–1920, https://doi.org/10.1093/mnras/staf338
JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1921–1943, https://doi.org/10.1093/mnras/staf359
Investigating the influence of the radiative torque disruption on the size evolution of dust in the heliosphere
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1944–1962, https://doi.org/10.1093/mnras/staf369
On the origin of the Hercules group – I. Chemical signatures indicating the outer bar origin
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1963–1979, https://doi.org/10.1093/mnras/staf392
Constraining the phase shift of relativistic species in DESI BAOs
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 1980–2000, https://doi.org/10.1093/mnras/staf394
Gamma-ray burst empirical correlation between peak luminosity and peak energy in the ICMART model
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2001–2007, https://doi.org/10.1093/mnras/staf064
MOJAVE – XXII. Brightness temperature distributions and geometric profiles along parsec-scale active galactic nucleus jets
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2008–2030, https://doi.org/10.1093/mnras/staf343
Exoplanet transit candidate identification in TESS full-frame images via a transformer-based algorithm
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2031–2049, https://doi.org/10.1093/mnras/staf347
Joint cosmic density reconstruction from photometric and spectroscopic samples
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2050–2057, https://doi.org/10.1093/mnras/staf390
Type I X-ray burst emission reflected into the eclipses of EXO 0748−676
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2058–2074, https://doi.org/10.1093/mnras/staf395
Comparison between cycle-to-cycle variations in the coefficient of Joy’s law and covariance of rotation residuals and meridional motions of sunspot groups
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2075–2083, https://doi.org/10.1093/mnras/staf409
The large PAH sumanene: laboratory rotational spectroscopy and astronomical search
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2084–2088, https://doi.org/10.1093/mnras/staf421
Multiphysics framework for fast modelling of gamma-ray burst afterglows
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2089–2115, https://doi.org/10.1093/mnras/staf302
Lowest-mass X-ray selected AGNs in the Boötes field
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2116–2128, https://doi.org/10.1093/mnras/staf322
The formation, evolution, and disruption of star clusters with improved gravitational dynamics in simulated dwarf galaxies
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2129–2148, https://doi.org/10.1093/mnras/staf350
Multimessenger modelling of the Monogem pulsar halo
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2149–2160, https://doi.org/10.1093/mnras/staf374
Revisiting the observation–theory confrontation in high-frequency QPOs: a new QPO in NGC 5506, intermediate-mass black holes, and the crucial role of accretion state
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2161–2170, https://doi.org/10.1093/mnras/staf391
Autoregressive moving average modelling of TESS photometry of massive stars
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2171–2185, https://doi.org/10.1093/mnras/staf403
Temporal variability and obscuration effects in the X-ray emission of classical nova V339 Delphini (Nova Delphini 2013)
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2186–2203, https://doi.org/10.1093/mnras/staf420
Boosting H i-galaxy cross-clustering signal through higher order cross-correlations
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2204–2218, https://doi.org/10.1093/mnras/staf433
Probing the physical environment of the most high-redshift H2-DLAs through numerical models
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2219–2232, https://doi.org/10.1093/mnras/staf437
Synthetic spectroscopy for white dwarf classification: addressing label uncertainty and class imbalance
Monthly Notices of the Royal Astronomical Society, Volume 538, Issue 3, April 2025, Pages 2233–2244, https://doi.org/10.1093/mnras/staf448
