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Attributs	Valeurs
type	work Issue
Is Part Of	http://hub.abes.fr/oup/periodical/mnras/1997/volume_289
has manifestation of work	http://hub.abes.fr/oup/periodical/mnras/1997/volume_289/issue_4/m/print http://hub.abes.fr/oup/periodical/mnras/1997/volume_289/issue_4/m/web
Date Copyrighted	1997
Rights	© 1997 RAS
issue	4
is Is Part Of of	On the mass distribution in the Shapley Supercluster inferred from X-ray observations Further critical tests of stellar evolution by means of double-lined eclipsing binaries An updated precision estimate of the Hubble constant and the age and density of the Universe in the decaying neutrino theory High-redshift radio galaxies and quasars at submillimetre wavelengths: assessing their evolutionary status ROSAT observations of two ‘cooling flow’ EMSS galaxies Incorporating radiative cooling into a cosmological hydrodynamic code Is there really a supermassive black hole in M87? The relative distances to the Virgo, Fornax and Coma clusters of galaxies through the Dn-σ and the Fundamental Plane relations The supercluster-void network - II. An oscillating cluster correlation function The determination of time delays as an inverse problem - the case of the double quasar 0957+561 Radio-excess infrared galaxies: a new population of active galaxies? Optical, infrared and millimetre-wave properties of Vega-like systems - III. Models with thermally spiking grains Hα profile variations in the long-period Cepheid ℓ Carinae UBVRI photometry of the pulsations in V2116 Ophiuchi ≡ GX1+4 The history of star formation in the local disc from the G dwarf metallicity distribution Optical and H I studies of high- and intermediate-velocity gas towards Complex A Asymmetry of jets, lobe length and spectral index in quasars Reproducing superhumps and γ-shifts of SU UMa stars with SPH simulations The properties of the hot gas in galaxy groups and clusters from ID hydrodynamical simulations - I. Cosmological infall models 12C/13C ratios and Li abundances in C stars: evidence for deep mixing? The supercluster-void network - III. The correlation function as a geometrical statistic The cooling of oxygen—neon white dwarfs Occultations by Kuiper belt objects On the effects of dynamical evolution on the initial mass function of globular clusters CO mapping of the central regions of the globular clusters ω Cen and 47 lue On the role of magnetic fields in H I rotation curves

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