ESR EuroSafe Imaging and its role in promoting radiation protection - 6 years of success. [PDF]
Insights Imaging, 2021 Frija G +10 more
europepmc +2 more sources
Cumulative effective dose from recurrent CT examinations in Europe: proposal for clinical guidance based on an ESR EuroSafe Imaging survey. [PDF]
Eur Radiol, 2021 Frija G +5 more
europepmc +2 more sources
Inner dusty envelope of the AGB stars W Hydrae, SW Virginis, and R Crateris using SPHERE/ZIMPOL [PDF]
Astronomy & Astrophysics, 2020 Context. The asymptotic giant branch (AGB) marks the final evolutionary stage of stars with initial masses between ~0.8 and 8 M⊙. During this phase, stars undergo copious mass loss, which contributes significantly to the enrichment of the interstellar ...
T. Khouri +10 more
semanticscholar +1 more source
Dentists in action: a profession on-screen (1913-2013)
British Dental Journal, 2022 Background Fictional portrayals of dentists in feature films have remained largely unexamined to date. The aim of this review is consequently to catalogue and analyse available films produced by US entertainment industry that present 'dentists in action'.
Samuel Gierok +2 more
semanticscholar +1 more source
Large-scale magnetic topologies of late M dwarfs★: Magnetic topologies of late M dwarfs [PDF]
, 2010 We present here the final results of the first spectropolarimetric survey of a small sample of active M dwarfs, aimed at providing observational constraints on dynamo action on both sides of the full-convection threshold (spectral type M4).
J. Morin +5 more
semanticscholar +1 more source
Large-scale magnetic topologies of late M dwarfs⋆ [PDF]
, 2008 We present here the final results of the first spectropolarimetric survey of a small sample of active M dwarfs, aimed at providing observational constraints on dynamo action on both sides of the full-convection threshold (spectral type M4).
J. Morin +15 more
semanticscholar +1 more source
Search of X-ray emission from roAp stars: the case of γ Equulei [PDF]
, 2011 The detection of X-ray emission from Ap stars can be an indicator for the presence of magnetic activity and dynamo action, provided different origins for the emission, such as wind shocks and close late-type companions, can be excluded. Here we report on
B. Stelzer +4 more
semanticscholar +1 more source
ALMA sub-mm maser and dust distribution of VY Canis Majoris [PDF]
, 2014 Aims. Cool, evolved stars have copious, enriched winds. Observations have so far not fully constrained models for the shaping and acceleration of these winds.
A. M. S. Richards +27 more
semanticscholar +1 more source
A surprisingly large asymmetric ejection from Mira A [PDF]
Astronomy & AstrophysicsStars with masses between roughly 1 and 8 M_⊙ end their lives on the asymptotic giant branch (AGB), when intense mass loss takes place, with major consequences for the chemical evolution of the universe.
T. Khouri +8 more
semanticscholar +1 more source
LABOCA 870 μm dust continuum mapping of selected infrared-dark cloud regions in the Galactic plane [PDF]
, 2012 Context. Imaging surveys of dust emission at (sub)millimetre wavelengths provide a powerful tool for studying molecular clouds and the early stages of star formation. Aims.
O. Miettinen
semanticscholar +1 more source