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Attributs	Valeurs
type	work Issue
Is Part Of	http://hub.abes.fr/oup/periodical/mnras/2010/volume_403
has manifestation of work	http://hub.abes.fr/oup/periodical/mnras/2010/volume_403/issue_4/m/web http://hub.abes.fr/oup/periodical/mnras/2010/volume_403/issue_4/m/print
Date Copyrighted	2010
Rights	© 2010 The Author. Journal compilation © 2010 RAS © 2010 The Authors. Journal compilation © 2010 RAS
issue	4
is Is Part Of of	UBV(RI)CJHK observations of Hipparcos-selected nearby stars A long-period planet orbiting a nearby Sun-like star The variation of the galaxy luminosity function with group properties Dynamical erosion of asteroid groups in the region of the Phocaea family Observations of the quiescent X-ray transients GRS 1124-684 (=GU Mus) and Cen X-4 (=V822 Cen) taken with ULTRACAM on the VLT Global collapses and expansions in star-forming clouds Optical polarization observations in the Scorpius region: NGC 6124 X-ray groups and clusters of galaxies in the Subaru-XMM Deep Field Effect of plasma composition on the interpretation of Faraday rotation Local kinematics and the local standard of rest A compact pulsar wind nebula model of the γ-ray-loud binary LS I +61○303 The role of r-mode damping in the thermal evolution of neutron stars A resonance model with magnetic connection for 3:2 HFQPO pairs in black hole binaries The axis of evil - a polarization perspective Pulsations in the atmosphere of the roAp star HD 24712 - II. Theoretical models 3D models of radiatively driven colliding winds in massive O + O star binaries - II. Thermal radio to submillimetre emission 3D models of radiatively driven colliding winds in massive O + O star binaries - III. Thermal X-ray emission A joint Chandra and XMM-Newton view of Abell 3158: a massive off-centre cool gas clump as a robust diagnostic of a merger stage The observable effects of tidally induced warps in protostellar discs Hierarchical models of high-redshift galaxies with thermally pulsing asymptotic giant branch stars: comparison with observations Observation and modelling of main-sequence star chromospheres - X. Radiative budgets on Gl 867A and AU Mic (dM1e), and a two-component model chromosphere for Gl 205 (dM1) Detailed characterization of Hβ emission line profile in low-z SDSS quasars Tight constraints on the existence of additional planets around HD 189733 Convolution- and deconvolution-based estimates of galaxy scaling relations from photometric redshift surveys popstar evolutionary synthesis models II: optical emission-line spectra from giant H ii regions A multifrequency method based on the matched multifilter for the detection of point sources in CMB maps Study of sdO models: mode trapping On the overconcentration problem of strong lensing clusters Modelling the spectral behaviour of night skylight close to artificial light sources More on lensing by a cosmological constant Erratum: A 3D dynamical model of the colliding winds in binary systems An application of Galactic parallax: the distance to the tidal stream GD-1 Note on galaxy catalogues in UHECR flux modelling Ionized gas in the starburst core and halo of NGC 1140 New insight into the relation between star formation activity and dust content in galaxies Study of a homogeneous QSO sample: relations between the QSO and its host galaxy Mesoscale optical turbulence simulations at Dome C: refinements Radiative transfer in disc galaxies - IV. The effects of dust attenuation on bulge and disc structural parameters Ionized gas outflow in the isolated S0 galaxy NGC 4460 The slope of the mass profile and the tilt of the Fundamental Plane in early-type galaxies The nature of the Sloan Digital Sky Survey galaxies in various classes based on morphology, colour and spectral features - III. Environments The velocity function of gas-rich galaxies Large-scale structure and dynamics of the most X-ray luminous galaxy cluster known - RX J1347−1145 Second-order Lagrangian perturbation theory initial conditions for resimulations Hydrodynamical N-body simulations of coupled dark energy cosmologies The rotational structure of methanol and its excitation by helium Gas dynamics of the central few parsec region of NGC 1068 fuelled by the evolving nuclear star cluster

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