Results 81 to 90 of about 97,661 (176)
Spherical Accretion in the Schwarzschild Spacetime in the Newtonian Analogous Construct
The velocity-dependent Newtonian analogous potentials (NAPs) corresponding to general relativistic (GR) spacetimes accurately capture most of the relativistic features, including all classical tests of GR, effectively representing spacetime geometries in
Shubhrangshu Ghosh +4 more
doaj +1 more source
Neutron stars harboring a primordial black hole: Maximum survival time. [PDF]
Baumgarte TW, Shapiro SL.
europepmc +1 more source
A Streamer Driving Misalignment in the Circumtriple Disk of GW Ori
GW Ori is a triple stellar system with a disk featuring three misaligned dust rings. We present Atacama Large Millimeter/submillimeter Array molecular line data of CO isotopologues, revealing a streamer feeding the disk in ^12 CO and ^13 CO.
Maria Galloway-Sprietsma +7 more
doaj +1 more source
There have been many research works involving mass transfer in stellar binaries, all of which are limited to certain systems with specific binary parameters.
Bushra Ata Ali +2 more
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Mass Transfer in Mira-Type Binaries
Detached, symbiotic binaries are generally assumed to interact via Bondi-Hoyle-Littleton (BHL) wind accretion. However, the accretion rates and outflow geometries that result from this mass-transfer mechanism cannot adequately explain the observations of
Mohamed S., Podsiadlowski Ph.
doaj +1 more source
Accretion onto a small black hole at the center of a neutron star. [PDF]
Richards CB, Baumgarte TW, Shapiro SL.
europepmc +1 more source
Spinning supermassive black holes (BHs) in active galactic nuclei magnetically launch relativistic collimated outflows, or jets. Without angular momentum supply, such jets are thought to perish within 3 orders of magnitude in distance from the BH, well ...
Aretaios Lalakos +6 more
doaj +1 more source
Silicon isotope constraints on terrestrial planet accretion. [PDF]
Onyett IJ +5 more
europepmc +1 more source
On Disk Formation around Isolated Black Holes via Stream Accretion
We investigate accretion onto an isolated black hole from uniform winds. If the winds are directed toward the black hole, then the accretion process can be well described by the classical Bondi–Hoyle–Lyttleton or BHL accretion.
Priyesh Kumar Tripathi +2 more
doaj +1 more source
MESA-QUEST: Tracing the Formation of Direct Collapse Black Hole Seeds via Quasi-stars
The origin of the first supermassive black holes (SMBHs) observed at redshifts z ≥ 9 remains one of the most challenging open questions in astrophysics.
Andrew D. Santarelli +5 more
doaj +1 more source

