Results 21 to 30 of about 118,894 (281)
Magnetospheric accretion on the fully-convective classical T Tauri star DN Tau [PDF]
, 2013 The MaPP project is supported by the funding agencies of CFHT and TBL (through the allocation of telescope time) and by INSU/CNRS in particular, as well as by the French ‘Agence Nationale pour la Recherche’ (ANR).
Menard, F +28 more
core +1 more source
, 2021 In the two-phase scenario of galaxy formation, a galaxy's stellar mass growth is first dominated by in-situ star formation, and subsequently by accretion. We analyse the radial distribution of the accreted stellar mass in ~500 galaxies from the hydrodynamical cosmological simulation Magneticum.
Remus, Rhea-Silvia, Forbes, Duncan A.
openaire +2 more sources
The X-ray position and optical counterpart of the accretion-powered millisecond pulsar XTE J1814−338 [PDF]
, 2005 We report the precise optical and X-ray localization of the 3.2 ms accretion-powered X-ray pulsar XTE J1814-338 with data from the Chandra X-Ray Observatory as well as optical observations conducted during the 2003 June discovery outburst.
Wang, Zhongxiang +9 more
core +1 more source
Full-scale runback ice: accretion and aerodynamic study [PDF]
, 2010 The runback ice phenomenon is well-known for anti-icing or de-icing systems when the system is not evaporating 100% of the water impinging the surface.
Alegre, Nathalie
core +3 more sources
Temperaments of young stars : rapid mass accretion rate changes in T Tauri and Herbig Ae stars [PDF]
, 2014 Funding: JSV would like to thank the UK Science and Technologies Facility Council (STFC) and the Northern Ireland Department of Culture Arts and Leisure (DCAL) for financial support.
G. Costigan +10 more
core +1 more source
TERRAIN TECTONICS OF THE CENTRAL ASIAN FOLDED BELT
Геодинамика и тектонофизика, 2015 The terrain analysis concept envisages primarily a possibility of approximation of fragments / terrains of various geodynamic settings which belong to different plates. The terrain analysis can supplement the theory of plate tectonics in solving problems
M. M. Buslov
doaj +1 more source
Accretion-powered stellar winds. III. spin-equilibrium solutions [PDF]
, 2008 We compare the stellar wind torque calculated in a previous work (Paper II) to the spin-up and spin-down torques expected to arise from the magnetic interaction between a slowly rotating (∼10% of breakup) pre-main-sequence star and its accretion disk ...
Sean P. Matt (21829835) +1 more
core +4 more sources
An automatic multi-stepping approach to aircraft ice prediction [PDF]
, 2007 Flying an aircraft in icing conditions may seriously degrade its aerodynamical performance and threaten the flight safety. Over the years, new technologies and improved procedures have limited the potential risks caused by aircraft icing. Experimental
Verdin, Patrick G.
core +6 more sources
Self-Similar Solution of Hot Accretion Flow with Anisotropic Pressure
Universe, 2019 For the accretion flow in extremely low-luminosity active galactic nuclei, such as our Galactic center (Sgr A*) and M 87, the collisional mean-free path of ions may be much larger than its gyroradius.
De-Fu Bu, Pei-Yao Xu, Bo-Cheng Zhu
doaj +1 more source
Universe, 2019 For systems with extremely low accretion rate, such as Galactic Center Sgr A* and M87 galaxy, the ion collisional mean free path can be considerably larger than its Larmor radius. In this case, the gas pressure is anisotropic to magnetic field lines.
Hui-Hong Deng, De-Fu Bu
doaj +1 more source