Results 31 to 40 of about 127,865 (133)

The GRAVITY Young Stellar Object survey IV. The CO overtone emission in 51 Oph at sub-au scales [PDF]

open access: yes, 2020
51 Oph is a Herbig Ae/Be star that exhibits strong near-infrared CO ro-vibrational emission at 2.3 micron, most likely originating in the innermost regions of a circumstellar disc. We aim to obtain the physical and geometrical properties of the system by spatially resolving the circumstellar environment of the inner gaseous disc.
arxiv   +1 more source

Risk of temporomandibular joint effusion related to magnetic resonance imaging signs of disc displacement [PDF]

open access: yes, 2009
Background: It has been suggested that TMJ effusion may represent an inflammatory response to a dysfunctional disc-condyle relationship. The purpose of the present study was to evaluate whether the status of the disc in the temporomandibular joint, as ...
Bosco, Mario   +3 more
core  

Dust Spreading in Debris Discs: Do Small Grains Cling on to Their Birth Environment? [PDF]

open access: yes, 2019
Debris discs are dusty belts of planetesimals around main-sequence stars, similar to the asteroid and Kuiper belts in our solar system. The planetesimals cannot be observed directly, yet they produce detectable dust in mutual collisions. Observing the dust, we can try to infer properties of invisible planetesimals.
arxiv   +1 more source

Rotating relativistic thin disks as sources of charged and magnetized Kerr-NUT spacetimes [PDF]

open access: yesInt. J. Mod. Phys. D, Vol. 18, No. 9 (2009), pags. 1461-1481, 2008
A family of models of counterrotating and rotating relativistic thin discs of infinite extension based on a charged and magnetized Kerr-NUT metric are constructed using the well-known "displace, cut and reflect" method extended to solutions of vacuum Einstein-Maxwell equations.
arxiv   +1 more source

Hydroelastic effects during the fast lifting of a disc from a water surface [PDF]

open access: yesJournal of Fluid Mechanics. Vol. 869, pp. 726-751, June 2019, 2018
Here we report the results of an experimental study where we measure the hydrodynamic force acting on a plate which is lifted from a water surface, suddently starting to move upwards with an acceleration much larger than gravity. Our work focuses on the early stage of the plate motion, when the hydrodynamic suction forces due to the liquid inertia are ...
arxiv   +1 more source

Dynamic Behaviour of a Two-Stage Cycloidal Speed Reducer of a New Design Concept [PDF]

open access: yes, 2018
Traditional cycloidal speed reducers (with two cycloid discs per one stage, mutually turned by an angle of 180°) are well known for their remarkable dynamic stability.
Miloš Matejić   +2 more
core   +2 more sources

Formation of rings in galactic discs by infalling small companions [PDF]

open access: yes, 1996
We use N-body simulations to study the formation of rings in a disc galaxy by the impact of a small spherical companion. Both barred and nonbarred target discs are considered. We discuss the effect of the properties of the target disc (distribution of mass in the disc, velocity dispersion, etc.) as well as of the mass and orbit of the companion on the ...
arxiv   +1 more source

FasL Expression in Articular Discs of Human Temporomandibular Joint and Association with Osteoarthrosis [PDF]

open access: yes, 2013
Background Apoptosis is a programme of cell death which does not induce an inflammatory response. Recent previous research has suggested a correlation between temporomandibular internal derangement and apoptosis.
Alanis, Luciana Reis Azevedo   +9 more
core   +2 more sources

The high frequency flexural ultrasonic transducer for transmitting and receiving ultrasound in air [PDF]

open access: yes, 2020
Flexural ultrasonic transducers are robust and low cost sensors that are typically used in industry for distance ranging, proximity sensing and flow measurement.
Dixon, Steve M.   +2 more
core   +3 more sources

Galactic seismology: the evolving "phase spiral" after the Sagittarius dwarf impact [PDF]

open access: yes, 2020
In 2018, the ESA \Gaia\ satellite discovered a remarkable spiral pattern ("phase spiral") in the $z-V_z$ phase plane throughout the solar neighbourhood, where $z$ and $V_z$ are the displacement and velocity of a star perpendicular to the Galactic disc.
arxiv   +1 more source

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