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Quasilinear Approach of the Whistler Heat-Flux Instability in the Solar Wind
Free accessArXiv | 2019| -
Footprints in the sand: What can globular clusters tell us about NGC 4753 past?
British Library Online Contents | 2015| -
Mass-loss from advective accretion disc around rotating black holes
British Library Online Contents | 2015| -
Planetesimal formation in self-gravitating discs – dust trapping by vortices
British Library Online Contents | 2015| -
Interpreting broad emission-line variations – II. Tensions between luminosity, characteristic size, and responsivity
British Library Online Contents | 2015| -
Unified dark matter: constraints from galaxies and clusters
British Library Online Contents | 2015| -
Local and global aspects of the linear MRI in accretion discs
British Library Online Contents | 2015| -
The link between accretion mode and environment in radio-loud active galaxies
British Library Online Contents | 2015| -
Searching for gas giant planets on Solar system scales – a NACO/APP L′-band survey of A- and F-type main-sequence stars
British Library Online Contents | 2015| -
X-ray emission from the giant magnetosphere of the magnetic O-type star NGC 1624-2
British Library Online Contents | 2015| -
GHASP: an Hα kinematic survey of spiral galaxies – X. Surface photometry, decompositions and the Tully–Fisher relation in the Rc band★
British Library Online Contents | 2015| -
A systematic synchro-curvature modelling of pulsar γ-ray spectra unveils hidden trends
British Library Online Contents | 2015| -
Probing the nature of the pre-merging system Hickson Compact Group 31 through integral field unit data★
British Library Online Contents | 2015| -
The excitation mechanism of H2 in bipolar planetary nebulae
British Library Online Contents | 2015|
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