Results 131 to 140 of about 491,052 (394)
Long-term variability of low-mass X-ray binaries
We consider modulations of mass captured by the compact object from the companion star’s stellar wind in Low Mass X-ray Binaries with late type giants. Based on 3D simulations with two different hydrodynamic codes used Lagrangian and Eulerian approaches –
Filippova E. +2 more
doaj +1 more source
The transiting dust clumps in the evolved disc of the Sun-like UXor RZ Psc [PDF]
RZ Psc is a young Sun-like star, long associated with the UXor class of variable stars, which is partially or wholly dimmed by dust clumps several times each year.
Grant M. Kennedy +6 more
doaj +1 more source
Magnetically warped discs in close binaries
We demonstrate that measurable vertical structure can be excited in the accretion disc of a close binary system by a dipolar magnetic field centred on the secondary star.
Applegate +40 more
core +1 more source
Dissipative advective accretion disc solutions with variable adiabatic index around black holes [PDF]
We investigated accretion on to black holes in presence of viscosity and cooling, by employing an equation of state with variable adiabatic index and multi-species fluid.
Rajiv Kumar, I. Chattopadhyay
semanticscholar +1 more source
Naked cuticle is essential for Drosophila wing development beyond Wingless signaling
Naked cuticle (Nkd), a Wnt signaling inhibitor, assumes extensive roles in Drosophila wing development. Overexpressing Nkd causes smaller, crumpled wings, while also perturbing multiple signaling pathways and developmental genes. A specific region (R1S) is critical for Nkd's function as a signaling integrator, offering new insights for studying its ...
Rui Wang, Ping Wang
wiley +1 more source
Disk precession of V603 Aql in 2001-2002
The rezults of the novalike variable V603 Aql photometric observations performed by Russian-Turkish telescope RTT150 during 11 nights of 2001 - 2002 are presented.
V. F. Suleimanov +7 more
doaj +1 more source
Many statistical properties of X-ray aperiodic variability from accreting compact objects can be explained by the propagating fluctuations model applied to the accretion disc.
Ingram, Adam +2 more
core +2 more sources
The Comptonization of accretion disc X-ray emission: consequences for X-ray reflection and the geometry of AGN coronae [PDF]
We consider the Comptonisation of the photons that make up the relativistically blurred reflection that is commonly detected from the accretion discs of AGN by the coronae of energetic particles believed to give rise to the powerful X-ray continua by the
D. Wilkins, L. Gallo
semanticscholar +1 more source
KHS‐Cnd peptide is able to impair biofilm formation and disaggregate mature biofilms in Acinetobacter baumannii clinical isolates. Differences in extracellular metabolites reflect changes in biofilm metabolism due to KHS‐Cnd treatment. Among the differentially represented extracellular metabolites upon KHS‐Cnd treatment, the significantly altered ...
Fernando Porcelli +9 more
wiley +1 more source
The formation of planets by disc fragmentation
I discuss the role that disc fragmentation plays in the formation of gas giant and terrestrial planets, and how this relates to the formation of brown dwarfs and low-mass stars, and ultimately to the process of star formation.
Stamatellos Dimitris
doaj +1 more source

