「accretion」の共起表現(1語右で並び替え)

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共起表現

「accretion」の共起表現一覧(1語右で並び替え)

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tary to Lord Burghley, and became (by steady	accretion) a substantial landowner.
Predicting patterns of continental	accretion and breakup of continents and supercontinent
A well-known specialist in theory of	accretion and in astrophysics of x-ray binaries, toget
have a "supercontinent oscillation", with an	accretion and breakup wavelength of ~500 million years
Use of the term	accretion disc for the protoplanetary disc thus leads
nnot produce its own magnetic field, but its	accretion disc can.
The captured material forms a gaseous	accretion disc and spirals inwards to ultimately fall
and Horne, K. (1997) Spiral structure in the	accretion disc of IP Pegasi, Monthly Notices of the Ro
For example, if a jet originates in the	accretion disc, its plasma is likely to have electron-
mentum, which is very likely generated by an	accretion disc.
ntral object (such as a black hole), and the	accretion disc.
	Accretion discs around many stellar objects are able t
While it is not known exactly how	accretion discs manage to produce jets, they are thoug
radiation hydrodynamics and plasma physics,	accretion discs, the evolution of stars, the dynamics
terial from the K0 star is transferred to an	accretion disk surrounding the unidentified primary st
ins uncertain whether the white dwarf has an	accretion disk formed by this material.
The secondary, more massive star has an	accretion disk due to this mass transfer.
nova are caused when matter from a ring-like	accretion disk becomes unstable.
ield of the white dwarf is too strong for an	accretion disk to form.
hole is the source of X-Ray flareups due to	accretion disk that surrounds it.
This	accretion disk blocks our view of the secondary star,
om a true eclipse (0.514195 d period) of the	accretion disk at fairly high binary inclination.
m, a dust solution could be used to model an	accretion disk around a massive object; however, no su
y material flowing into the black hole in an	accretion disk created a vigorous outflow of gas from
flow of gas is fairly thin and slow, so the	accretion disk remains relatively cool, and little gas
er of the galaxy by jets associated with the	accretion disk around the supermassive black hole.
From observations, a twisted	accretion disk, in retrograde precession, modulates th
In certain sense it behaves like a thick	accretion disk, except that it also has radial velocit
co-discovery of spiral waves in a solar-size	accretion disk, pioneering analysis determining mass r
iodic surge of influx from the white dwarf's	accretion disk, caused by instability in the disk itse
t dwarf novae result from instability in the	accretion disk, when gas in the disk reaches a critica
thin disk around the black hole, known as an	accretion disk.
stripped by a white dwarf in the form of an	accretion disk.
uring eclipse and superhumps produced by the	accretion disk.
object draws matter from its partner via an	accretion disk.
lieved associated with the precession of the	accretion disk.
Structure of	accretion disks around AGN
Diskoseismology is the behavioral study of	accretion disks surrounding black holes.
Water masers are useful to observe nuclear	accretion disks in active galaxies.
oped the general relativistic theory of thin	accretion disks around black holes, and using this the
ed gas surrounding neutron stars, black hole	accretion disks or at the edge of ultra-compact HII re
ing of astrophysics including the model that	accretion disks are supported by magnetic fields, that
Non-magnetic systems exhibit full	accretion disks, while strongly magnetic systems exhib
He works on the theory of	accretion disks, with particular application to the fo
odes in stars and different instabilities in	accretion disks.
rotation, and probe quasars including their	accretion disks.
Massive amounts of	accretion, due in large part to the jetty system at th
atmosphere of a planet that did not form by	accretion during the formation of the planet's sun.
he shock and the innermost sonic point of an	accretion flow becomes hot due to sudden reduction of
n the context of neutron star and black hole	accretion for compact objects traveling through the in
lanet's condensation from a solar nebula and	accretion from meteorites, as well as the formation of
This gradual	accretion has produced a complex plan and floor number
The lifetime of this high	accretion, high luminosity phase is on the order of de
It appears that	accretion in the early 1840s was followed by erosion i
rked increase in protein and decrease in fat	accretion in animals, in particular swine.
n and evaporation processes, thereby causing	accretion in water vapour and cloud cover, the primary
ranspiration and evaporation thereby causing	accretion in water vapor and cloud cover which are the
ranspiration and evaporation thereby causing	accretion in water vapour and cloud cover which are th
Standard Ice	Accretion Indicator (upside down)
The Ice	Accretion Indicator is an L-shaped piece of aluminium
minosities, distances, and the efficiency of	accretion into a "Schwarzschild throat" through the la
Protein turnover (also known as protein	accretion) is the balance between protein synthesis an
In astrophysics, the term	accretion is used for at least two distinct processes.
Slowing of the	accretion is caused by gravitational perturbations by
	Accretion is an atmospheric science term for when an i
The runaway	accretion lasts between 10,000 and 100,000 years and e
g how planets form and supports solar nebula	accretion mode.
haeton hypothesis has been superseded by the	accretion model.
This may be due to the	accretion of metal-poor circumstellar gas.
It represents the Late Cretaceous to Eocene	accretion of what is known as the "Insular Superterran
cataclysmic outbursts appear to be caused by	accretion of material from the M-star to the white dwa
The most obvious is by slow	accretion of matter starting from a black hole of stel
ted (usually in the form of heat) during the	accretion of such an object from material falling from
he neutron star is caused by the capture and	accretion of matter from the stellar wind of the super
orial ridge was then produced by collisional	accretion of this ring.
the origin of M94's outer disk including the	accretion of a satellite galaxy or the gravitational i
ed the decision in Handly's Lessee regarding	accretion of new land and held that 1792 low-water mar
l bone is formed within the Dermis; Grows by	accretion only; outer portion of the bone depositing m
caused by magnetic activity, or possibly by	accretion onto a white dwarf companion.
s, the formation of low and high mass stars,	accretion onto neutron stars, and Compton-heated winds
and Nikolay I. Shakura developed a model of	accretion onto black holes, from a disk, and he has pr
gely invisible, being covered by superficial	accretion or infill.
ing of planetesimals tended to dominate over	accretion, preventing the formation of planet-sized bo
However, the process of coastal	accretion proceeded and a salt marsh developed, leavin
as been predicted in some models of the core	accretion process.
planet was then created using a stellar dust	accretion program based on the mass of each star.
The	accretion rate therefore becomes .
can undergo surface nuclear burning when the	accretion rate exceeds a certain limit.
Mass	accretion rates for these objects are estimated to be
In the nebular theory,	accretion refers to the collision and sticking of cool
From this time, the accommodation grew by	accretion so that by 1867 the carriage department was
(Tables of erosion and	accretion, started by G.O. Case have been maintained b
enerated by high velocity particles from the	accretion stream forming a shock front as they fall on
Infalling gas forms an	accretion stream, following the dipole magnetic field
ite of processes like galaxy mergers and gas	accretion that might be expected to increase the scatt
Due to erosion and	accretion, the islands in the lower Mississippi are in
, icy) and the other "dry" (or rocky), whose	accretion was terminated by the formation of Jupiter.

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「accretion」の共起表現一覧(1語右で並び替え)