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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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cyclongenesis<br />

air masses along fronts. According to the structure<br />

of temperature <strong>and</strong> pressure, a cyclone can<br />

be classified as a barotropic cyclone (cold cyclone<br />

<strong>and</strong> warm cyclone), a baroclinic cyclone,<br />

or a neutral cyclone. Based on the distribution<br />

of geography, it can be classified as an extratropical<br />

cyclone, subtropic cyclone, or tropical<br />

cyclone. Since its lower level convergence can<br />

cause ascending air motion, cyclones are often<br />

accompanied by clouds <strong>and</strong> rain.<br />

cyclongenesis A development of synopticscale<br />

weather disturbances.<br />

cyclotron damping <strong>and</strong> instability In a collisionless<br />

plasma, damping or instability associated<br />

with then=±1 resonance, of importance<br />

in space physics <strong>and</strong> astrophysics as a mechanism<br />

of pitch-angle scattering of charged particles.<br />

See resonant damping <strong>and</strong> instability.<br />

cyclotron frequency See Larmor frequency.<br />

cyclotron radius See Larmor radius.<br />

Cygnus A Nearby (z = .056, about 200Mpc<br />

distant) active galaxy (3C 405) at RA19 h 59.4 m ,<br />

dec+40 ◦ 43 ′ which is a strong radio source, with<br />

radio jets that extend for about 50kpc in either<br />

direction. The closest <strong>and</strong> second strongest radio<br />

galaxy. Recently detected to have a small<br />

quasar-like core.<br />

© 2001 by CRC Press LLC<br />

Cygnus Loop Supernova remnant at RA20 h<br />

49 m 00 s dec+30 ◦ 30 ′ , 230 ′ × 160 ′ in extent. In<br />

the optical, a large filamentary loop, also strong<br />

in radio, visible in X-ray. Age of remnant is<br />

estimated at 20,000 years.<br />

Cygnus X1 (Cyg-X1) A binary system at<br />

RA 19 h 56 m 22 s .0, dec +35 ◦ 03 ′ 36 ′′ , at distance<br />

2.5 kpc, consisting of the O9.7 supergiant HDE<br />

226868 (Gies <strong>and</strong> Bolton 1986) <strong>and</strong> a compact<br />

object with an orbital period of 5.6 days. The<br />

mass of the unseen companion is significantly<br />

larger than 5M⊙, probably as large as 12M⊙.<br />

Cygnus X1 is the second brightest X-ray source<br />

in the sky, with X-ray emission exhibiting strong<br />

variability at time scales from milliseconds to<br />

years. It also radiates in γ -radiation. Because<br />

no theoretical models exist of compact degenerate<br />

(neutron) stars of mass exceeding 5M⊙,<br />

the system is taken as the prototype of a black<br />

hole binary. In this model, the compact object<br />

of mass ≈ 12M⊙ is the putative black hole, accreting<br />

mass from the hot supergiant companion<br />

star which has overflowed its Roche lobe<br />

through an accretion disk which thermally emits<br />

X-radiation. Cygnus X1 is also a radio source,<br />

with radio flux correlated to X-ray output. Also<br />

called 4U 1956+35.<br />

cynthion Of or pertaining to the moon.<br />

Cytherean Venusian, referring to the planet<br />

Venus.

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