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 +7 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. Richards +29 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
Hubble Space Telescope/WFPC2 and VLA Observations of the Ionized Gas in the Dwarf Starburst Galaxy NGC 4214 [PDF]
, 2000 We present new Hα and [O III] λ5007 narrowband images of the starbursting dwarf galaxy NGC 4214, obtained with the Wide Field and Planetary Camera (WFPC2) on board the Hubble Space Telescope (HST), together with VLA observations of the same galaxy.
J. Mackenty +4 more
semanticscholar +1 more source
A multifrequency study of the active star-forming complex NGC 6357 – I. Interstellar structures linked to the open cluster Pis 24 [PDF]
, 2011 We investigate the distribution of the gas (ionized, neutral atomic and molecular), and interstellar dust in the complex star forming region NGC6357 with the goal of studying the interplay between the massive stars in the open cluster Pis24 and the ...
C. Cappa +6 more
semanticscholar +1 more source
Crisis Management Communications For Popular Culture Events
Event Management, 2019 The connection of popular culture with tourism lies on the activity of individuals to travel to specific destinations mainly because of popular culture, events and themes existing in these specific areas (Miller & Washington, 2007).
N. Pappas
semanticscholar +1 more source