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Attributs	Valeurs
type	work Issue
Is Part Of	http://hub.abes.fr/oup/periodical/mnras/2010/volume_404
has manifestation of work	http://hub.abes.fr/oup/periodical/mnras/2010/volume_404/issue_1/m/web http://hub.abes.fr/oup/periodical/mnras/2010/volume_404/issue_1/m/print
Date Copyrighted	2010
Rights	© 2010 The Author. Journal compilation © 2010 RAS © 2010 The Authors. Journal compilation © 2010 RAS © 2010 RAS
issue	1
is Is Part Of of	Testing standard cosmology with large-scale structure On the exclusion of intracluster plasma from active galactic nuclei-blown bubbles Modelling CO formation in the turbulent interstellar medium PG 1258+593 and its common proper motion magnetic white dwarf counterpart Gas, dust and stars in the SCUBA galaxy, SMM J02399−0136: the EVLA reveals a colossal galactic nursery Discovery of Compton-thick quasars in the Sloan Digital Sky Survey Cosmological constraints from the clustering of the Sloan Digital Sky Survey DR7 luminous red galaxies Magnetic field regulated infall on the disc around the massive protostar Cepheus A HW2 Optical turbulence vertical distribution with standard and high resolution at Mt Graham HE 0230−4323 revisited: a new rapidly pulsating sdB star Finite thin disc models of four galaxies in the Ursa Major cluster: NGC 3877, NGC 3917, NGC 3949 and NGC 4010 There was movement that was stationary, for the four-velocity had passed around Improving PSF modelling for weak gravitational lensing using new methods in model selection Eccentricity pumping of a planet on an inclined orbit by a disc Slow m= 1 instabilities of softened gravity Keplerian discs First overtone CO bands in the giant component of RS Ophiuchi: the 12C/13C ratio in 2008 The rotational excitation of HCN and HNC by He: new insights on the HCN/HNC abundance ratio in molecular clouds The radio properties of a complete, X-ray selected sample of nearby, massive elliptical galaxies Dynamic emission properties of pulsars B0943+10 and B1822-09 - I. Comparison, and the discovery of a ‘Q’-mode precursor Interstellar extinction and polarization - a spheroidal dust grain approach perspective Exploring S-type orbits in the Pluto-Charon binary system Monthly Notices Letters Thermomagnetic instability in hot discs Abundances, masses and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in ΛCDM cosmologies Constraints on star-forming galaxies at z≥ 6.5 from HAWK-I Y-band imaging of GOODS-South Near-infrared dust and line emission from the central region of Mrk 1066: constraints from Gemini NIFS Photoionized gas in hydrostatic equilibrium: the role of gravity A multifrequency study of the large radio galaxies 3C46 and 3C452 Wave angular momentum and the evolution of planetary rings Prograde rotation of protoplanets by accretion of pebbles in a gaseous environment SN 2008iy: an unusual Type IIn Supernova with an enduring 400-d rise time In-depth studies of the NGC 253 ULXs with XMM-Newton: remarkable variability in ULX1, and evidence for extended coronae Near-infrared observations of nova V574 Puppis (2004) On merger bias and the clustering of quasars A model for saturation correction in meteor photometry UBVRI observations of the flickering of RS Ophiuchi at quiescence OH and H2O masers towards the star-forming region S140-IRS1 Limitations of model-fitting methods for lensing shear estimation 29 glitches detected at Urumqi Observatory Self-heating and its possible relationship to chromospheric heating in slowly rotating stars Astrophotonic spectroscopy: defining the potential advantage HD 209621: abundances of neutron-capture elements Galaxy And Mass Assembly (GAMA): the input catalogue and star-galaxy separation Weak lensing forecasts for dark energy, neutrinos and initial conditions Dust attenuation in the rest-frame ultraviolet: constraints from star-forming galaxies at z ∼ 1 Modelling stellar coronae from surface magnetograms: the role of missing magnetic flux The substructure hierarchy in dark matter haloes LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters at z= 0.2 A model for the cosmological evolution of low-frequency radio sources

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