「PULSAR」の共起表現(1語右で並び替え)

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共起表現

「PULSAR」の共起表現一覧(1語右で並び替え)

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3C58 or 3C 58 is a	pulsar and surrounding synchrotron nebula within the
f the pathfinder experiment was to be the Crab	Pulsar and Crab Nebula, and the Cygnus X-1 high mass
onal effects of the planet on the orbit of the	pulsar and white dwarf had been measured, giving an e
PSR B1509-58 is a	pulsar approximately 17,000 light-years away in the c
PSR B1828-10 is a	pulsar approximately 11,812 light-years away in the c
terplanetary Scintillation Array (IPS Array or	Pulsar Array) was built at the Mullard Radio Astronom
ghts into the behaviour of a neutron star or a	pulsar, as well as in quantum theory in general.
rth mass) gas giant was announced orbiting the	pulsar at a distance of about 40 AU.
The modern history of the Crab	Pulsar begins with the identification of the central
SAS-2 first detected Geminga, a	pulsar believed to be the remnant of a supernova that
s that magnetars are not merely a rare type of	pulsar but may be a (possibly reversible) phase in th
erhaps even more so than their more well known	pulsar counterparts.
gnal turned out to be radio emissions from the	pulsar CP1919 (the first one recognized as such).
r were studying what they thought was a binary	pulsar, determined that a third object was needed to
acker, studying what they thought was a binary	pulsar, determined that a third object was needed to
It is notable for being the first radio	pulsar ever discovered (in July 1967 by Jocelyn Bell
1+4, which was the first slowly rotating X-ray	pulsar found.
DAF DB250 10.2m / Wright	Pulsar Gemini for route 492.
s an active researcher within the Jodrell Bank	Pulsar Group.
This	pulsar has been the target of interest, because of a
clusters implies a much higher likelihood of a	pulsar having (or capturing) a giant companion star.
nova is Geminga ("Gemini gamma-ray source"), a	pulsar in the constellation Gemini.
Position of Crab	Pulsar in the Milky Way.
PSR J1903+0327 is a millisecond	pulsar in a highly eccentric binary orbit.
PSR J2007+2722 is a 40.8-hertz isolated	pulsar in the Vulpecula constellation, 5.3 kpc (17,00
Vela Supernova Remnant, located near the Vela	Pulsar in the constellation Vela.
Chandra observations of the	pulsar in 3C58 suggest that the matter in this collap
This	pulsar is distinguished by being the most stable natu
The	pulsar is unique in that it has a "bursting phase" wh
The Geminga	pulsar is closer (and also resulted from a supernova)
X-ray binary, HMXB - a high-mass X-ray binary,	Pulsar is an X-ray pulsar, radioBurst is a radio burs
An optical	pulsar is a pulsar which can be detected in the visib
	Pulsar is a 1981 arcade game created by Sega/Gremlin.
The Bursting	Pulsar is the only known X-ray pulsar that is also a
The	pulsar is about 1.8 solar mass and the companion is a
The mass of the	pulsar is estimated to be at least (1.88+/−0.13)
The	pulsar is located in a globular cluster of stars call
The	pulsar is accreting mass from this companion, resulti
the 30 Hz frequency of the Crab Nebula optical	pulsar is difficult for many people to see.
A	pulsar kick refers to the observed phenomenon that th
The cause of	pulsar kicks is unknown, but many astrophysicists bel
If true,	pulsar kicks would give us insight into the supernova
rmula is used with the second fastest-spinning	pulsar known, PSR J1748-2446ad (which rotates 716 tim
PSR J1748-2446ad is the fastest-spinning	pulsar known, at 716 Hz (period being 0.00139595482(6
48-2446ad in 2005, it was the fastest-spinning	pulsar known.
on of the Vela supernova remnant with the Vela	pulsar, made by astronomers at the University of Sydn
s of the companion is ~1 solar mass, while the	pulsar mass is unusually large at ~1.74 solar masses.
It is speculated that this	pulsar may in fact be a quark star.
peculate that gravitational radiation from the	pulsar might be detectable by LIGO.
wed the user to store information, following a	pulsar model released in 1982.
when they reported that they had discovered a	pulsar orbited by a planetary companion; this would h
The 1.24 second	pulsar period associated with Her X-1 is immediately
a astrophysics, Extragalactic radio astronomy,	Pulsar physics, Space radio spectroscopy, and Pulsar
1991, Andrew G. Lyne announced the first ever	pulsar planet discovered around PSR 1829-10.
very because of the retraction of the previous	pulsar planet, and questions about how pulsars could
lar planetary system discovered, and the first	pulsar planets discovered.
- although not confirmed - predating the 1992	pulsar planets found around PSR B1257+12 and main-seq
as later retracted, just before the first real	pulsar planets were announced.
	Pulsar planets are planets that are found orbiting pu
Although these	pulsar planets were not renamed, some have done it th
his method is similar to that used to discover	pulsar planets, except that the observations were in
tion to being the first confirmed discovery of	pulsar planets, the find is also generally considered
the fourth known extrasolar planet, excluding	pulsar planets.
ing car racer Glenn Seton who entered a Nissan	Pulsar powered Ralt RT4 late in the series.
planet planetary system around the millisecond	pulsar PSR 1257+12.
He discovered the first millisecond	pulsar, PSR B1937+21, which rotates at a rate far bey
is the second object known to be orbiting the	pulsar PSR B1257+12.
mutual inclination of the planets orbiting the	pulsar PSR B1257+12 had been determined by measuring
Jocelyn Bell Burnell, who discovered the first	pulsar PSR B1919+21 in 1967, relates that in the late
he planet is the innermost object orbiting the	pulsar PSR B1257+12, i.e. a pulsar planet.
In 1974, Hulse and Taylor discovered binary	pulsar PSR B1913+16, which is made up of a pulsar and
the team that discovered the first millisecond	pulsar, PSR B1937+21.
The	pulsar PSR B0950+08 seems to have come from a superno
of two planets and a possible third around the	pulsar PSR B1257+12.
e pulsars relied on two key characteristics of	pulsar pulses in order to distinguish pulsars from no
r Capital started a reinsurance company called	Pulsar Re.
	Pulsar runs on the Z80 microprocessor.
everal hundred km/s) of many pulsars, a single	pulsar scans the ISM rapidly, which results in changi
The second defining characteristic of	pulsar signals is the dispersion in frequency of an i
Vela X is a strong radio	pulsar source, that is also associated with a very st
tial data processing from the Parkes Multibeam	Pulsar Survey, which is the largest pulsar survey to
troacoustic music specializing in granular and	pulsar synthesis, author, and computer programmer.
abs contributed to the discovery of the binary	pulsar system PSR B1913+16 by Joseph Taylor and Russe
B1829-10 (often shortened to PSR 1829-10) is a	pulsar that is approximately 30,000 light-years away
rnice visits Marlowe's World to try and stop a	pulsar that threatens to destroy the Braxiatel Collec
nets discovered, and being discovered around a	pulsar, the planets were given the uppercase letters
The European	Pulsar Timing Array (EPTA) is a European collaboratio
It competes with the Australian and American	pulsar timing arrays, the Parkes Pulsar Timing Array
rames; lunar and interplanetary laser ranging;	pulsar timing experiments
d other colleagues have used this first binary	pulsar to make high-precision tests of general relati
s an ionized component, waves traveling from a	pulsar to Earth are dispersed, and thus pulsar survey
It was the first X-ray	pulsar to be discovered, and the third X-ray source t
the Alliance to deadly radiation from a nearby	pulsar until they finally surrender.
should not be confused with the isolated radio	pulsar, Vela X, which is a very different kind of obj
There are very few of these known: the Crab	pulsar was detected by stroboscopic techniques in 196
The Vela	pulsar was detected in 1977 at the Anglo-Australian O
Discovered in 1968, the	pulsar was the first to be connected with a supernova
The	pulsar was discovered in an ongoing L-band (1.4 GHz)
This	pulsar was discovered by Jason W. T. Hessels of McGil
the rotational frequency of a rotation-powered	pulsar, which usually decreases steadily due to braki
a neutron star with the properties of a radio	pulsar which emitted some magnetically-powered bursts
g voyage to the stars, and an encounter with a	pulsar whose pulse cycle is in phase with the brainwa
be that the X-ray emissions could be from the	pulsar wind nebula from a rapidly spinning pulsar, si
research group also discovered the first X-ray	pulsar with a rotation speed of four hundred revoluti
PSR J1748-2446ad, at 716 Hz, the	pulsar with the highest rotation speed.
Centaurus X-3 (4U 1118-60) is an X-ray	pulsar with a period of 4.84 seconds.
That is, a rapidly rotating	pulsar with a strong magnetic field, estimated at 101
SWIFT J1756.9-2508 is a millisecond	pulsar with a rotation frequency of 182 Hz (period of
The Crab nebula, and the Crab	Pulsar within it, is an intensive space X-ray source.

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