Volume 485 · Number 3 · 21 May 2019 3 · 21 · Number 485 Volume (print) 0035-8711 ISSN (online) 1365-2966 ISSN

Monthly Notices volume 485 • number 3 • 21 may 2019 • pages 2977–4463

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A one-dimensional hydrodynamic model for accretion, cooling, and heating of cooling, gas in dark model for accretion, one-dimensional hydrodynamic A Simulating the atomic and molecular content of and molecular content using probability molecular clouds the atomic Simulating A high-fidelityA of comparison code realization the Euclid TESS Titanium hidden in dust Titanium band up-conversion interferometer: first on-sky sensitivity on a single test arm interferometer: band up-conversion L Monthly Notices : a volumetric ray-marching tool for simulating microwave emission microwave for simulating tool a volumetric ray-marching : Three-dimensional supernova explosion simulations of 9-, 10-, 11-, 12-, and 13-M 12-, 11-, of 10-, simulations explosion supernova Three-dimensional 9-, The maps of and elemental abundance Doradus stars using gravito-inertial dipole modes and spectroscopy High-velocity absorption High-velocity emission in the spectrum and of supergiant HD 199478 γ Thyr Thyr Slowing the spins of cores stellar

Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone beyond of Cosmological simulations the need for ISM physics dwarfs: volume The gravitational force field of The gravitational the kinematics of in from force the Galaxy measured RR Lyrae Comprehensive abundance analysis of abundance giants red in the Comprehensive Numerical simulations of simulations motion of Numerical the controlled Emission line luminosity distributions of Seyfert 2 galaxies Cosmic-ray hydrodynamics: Alfvén-wave regulated transport regulated of rays Alfvén-wave cosmic hydrodynamics: Cosmic-ray = 0 z Unveiling the nature of Gemini multiconjugate adaptive optics system distortions optics system of adaptive the nature Gemini multiconjugate Unveiling Density distribution function of of turbulent a self-gravitating fluid in the context isothermal compressible Self-consistent redshift estimation using correlation estimation using correlation redshift Self-consistent No magnetars in ULXs No Spiral-arm instability – II. Magnetic destabilization Magnetic Spiral-arm instabilityII. – Forging new worlds: high-resolution synthetic galaxies with chained generative adversarial networks adversarial synthetic galaxies with high-resolution generative chained new worlds: Forging = 6 to = 6 to z Optical IFU spectroscopy of jet in NGC 300 Optical IFU spectroscopy a bipolar microquasar A code to Make Your Own Synthetic ObservaTIonS Own Synthetic (MYOSOTIS) Your Make to A code Rotational modulation in Rotational Towards a mid-infrared a mid-infrared Towards Mode switching and oscillations in PSR B1828–11 switching Mode Seismic modelling of early B-type BRITE – I. observed by pulsators A machine learningA machine artificial neural calibration abundance network of oxygen the strong-line WASP-92, WASP-93, and WASP-118: transit timing variations stability and long-term of the systems WASP-118: and WASP-93, WASP-92, ): The black hole X-ray transient J1357.2–0933 as seen with The black hole X-ray Swift B. M. B. 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Varga, J. 3446 3457 3430 3402 3409 3398 3386 3370 3378 3360 3352 3288 3296 3317 3334 3264 3642 3661 3681 3277 3600 3241 3248 3623 3558 3569 3224 3230 3588 3595 3499 3544 3514 3527 3042 3064 3076 3124 3153 3134 3580 3169 3203 3215 3185 3470 3476 3486 2977 3009 3024 3088 3097 3112 continued from outside back cover 3696 R. M. T. Connors et al.: Combining timing characteristics with physical broad-band spectral modelling of black hole X-ray binary GX 339–4 3715 D. M. Beronya, A. V. Karpova, A. Yu. Kirichenko, S. V. Zharikov, D. A. Zyuzin, Yu. A. Shibanov and A. Cabrera-Lavers: The ultracool helium- atmosphere white dwarf companion of PSR J0740+6620? 3721 G. Yang( ), W. N. Brandt, D. M. Alexander, C.-T. J. Chen( ), Q. Ni( ), F. Vito and F.-F. Zhu( ): Evident black hole-bulge coevolution in the distant 3738 D. J. Lagattuta et al.: Probing 3D structure with a large MUSE mosaic: extending the mass model of Frontier Field Abell 370 3761 K. Lund, K. Wood, D. Falceta-Gonçalves, B. Vandenbroucke, N. S. Sartorio, I. A. Bonnell, K. G. Johnston and E. Keto: Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H ii regions – spherically symmetric ionized accretion flows 3771 B. Vandenbroucke et al.: Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics THE BOARD OF EDITORS 3783 J. J. Davies, R. A. Crain, I. G. McCarthy, B. D. Oppenheimer, J. Schaye, M. Schaller and S. McAlpine: The gas fractions of dark matter haloes Editor-in-Chief: D. R. Flower, University of Durham hosting simulated ~L  galaxies are governed by the feedback history of their black holes Deputy Editor-in-Chief: A. R. King, University of Leicester 3794 I. del Moral-Castro et al.: Spotting the differences between active and non-active twin galaxies on kpc-scales: a pilot study 3816 I. Plotnikov and L. Sironi: The synchrotron maser emission from relativistic shocks in Fast Radio Bursts: 1D PIC simulations of cold pair plasmas P. Armitage, University of Colorado A. R. Liddle, Perimeter Institute for Theoretical Physics 3834 I. de Ruiter, J. van den Eijnden, A. Ingram and P. Uttley: A systematic study of the phase difference between QPO harmonics in black hole X-ray binaries E. Athanassoula, Laboratoire d'Astrophysique de Marseille T. Murphy, University of Sydney 3845 M. A. Dziełak, A. A. Zdziarski, M. Szanecki, B. De Marco, A. Nied´zwiecki and A. Markowitz: Comparison of spectral models for disc truncation M. J. Barlow, University College London C. D. Murray, Queen Mary, University of London in the hard state of GX 339–4 O. M. Blaes, University of California T. J. Pearson, California Institute of Technology A. J. Bunker, University of Oxford J. Schaye, Leiden Observatory 3857 A. E. L. Thomas et al.: Asteroseismic constraints on active latitudes of solar-type stars: HD 173701 has active bands at higher latitudes than the Sun C. Cacciari, INAF, Osservatorio Astronomico di Bologna A. Sozzetti, Osservatorio Astrofisico di Torino 3869 Z.-D. Shi and S. Liu: Origin of cosmic ray electrons and positrons R. F. Carswell, University of Cambridge A. N. Taylor, University of Edinburgh 3876 E. Gaidos, T. Hirano and M. Ansdell: Monitoring of the D doublet of neutral sodium during transits of two ‘evaporating’ planets A. Collier Cameron, University of St Andrews M. J. Ward, University of Durham 3887 L. Ohlin, F. Renaud and O. Agertz: Supernovae feedback propagation: the role of turbulence I. De Moortel, University of St Andrews A. L. Watts, University of Amsterdam 3895 T. J. Haworth and C. J. Clarke: The first multidimensional view of mass loss from externally FUV irradiated protoplanetary discs J. E. Drew, University of Hertfordshire S. D. M. White FRS, Max-Planck-Institut für Astrophysik 3909 A. Liu and P. Tozzi: Testing the rotation versus merger scenario in the Abell 2107 Downloaded from https://academic.oup.com/mnras/issue/485/3 by guest on 28 September 2021 M. W. Feast, University of Cape Town R. A. M. J. Wijers, University of Amsterdam 3919 B. Horowitz, S. Ferraro and B. D. Sherwin: Reconstructing small-scale lenses from the cosmic microwave background temperature fluctuations M. Gieles, University of Surrey D. M. Worrall, University of Bristol 3930 L. Drissen et al.: SITELLE: an Imaging Fourier Transform Spectrometer for the Canada–France–Hawaii Telescope 3947 C. A. Mason et al.: Inferences on the timeline of reionization at z ~ 8 from the KMOS Lens-Amplified Spectroscopic Survey Editorial office: The Editorial Office Manager, The Royal Astronomical Society, Burlington House, Piccadilly, London W1J 0BQ, UK 3970 A. A. Stanislavsky, K. Burnecki, J. Janczura, K. Niczyj and A. 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(ii) Bank transfer to Barclays Bank Plc, Oxford responsible sources Group Office, Oxford (bank sort code 20-65-18) (UK), overseas only ISSN: 0035-8711 (print); 1365-2966 (online) FSC® C007785 around 5480 BC as a result of the Solar system encounter with interstellar cloud Swift code BARC GB 22 (GB£ Sterling to account no. 70299332, © Mysid adapted from an original image by Roy Smits. This image 4446 M. D. Campbell-Brown: Solar cycle variation in radar meteor rates IBAN GB89BARC20651870299332; US$ Dollars to account no. is distributed under a CC BY-SA 3.0 Open Access licence, 4454 J. B. Biersteker and H. E. Schlichting: Atmospheric mass-loss due to giant impacts: the importance of the thermal component for 66014600, IBAN GB27BARC20651866014600; EU€ Euros to File:Pulsar_schematic.jpg, File:Pulsar_schematic.svg. hydrogen–helium envelopes