An Etymological Dictionary of Astronomy and Astrophysics
English-French-Persian

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 48 Search : galactic
active galactic nucleus (AGN)
  هسته‌ی ِ کهکشان ِ ژیرا   
haste-ye kahkašân-e žirâ

Fr.: noyau actif de galaxie   

A central region of an → active galaxy, which is a → light-year or less in diameter and has an abnormally high luminosity. The nucleus emits high energy radiation (→ gamma rays, → X-rays, → ultraviolet) and shows → variability over various time-scales, sometimes very short (hours to weeks). Emission line spectra reveal high velocity motions up to 104 km s-1. AGNs are divided into two main types. Type I refers to an AGN whose nucleus is visible (the spectra has both narrow and broad emission lines), while in type II AGN, the broad line region (BLR) is obscured and the lines are very narrow. This may be due either to the viewing angle or some intrinsic difference in structure. See also → broad-line region, → narrow-line region, → quasar.

active; → galactic; → nucleus.

apogalactic
  اپاکهکشانی   
apâkahkašâni

Fr.: apogalactique   

Of or pertaining to an → apogalacticon.

apo-; → galactic.

apogalacticon
  اپاکهکشان   
apâkahkašân

Fr.: apogalacticon   

The point at which a celestial body is farthest from the center of a galaxy; opposite of → perigalacticon.

From → apo- "away from, off" + galacticon, → galaxy.

From apâ, → apo-, + kahkašân, → galaxy.

circumgalactic medium (CGM)
  مدیم ِ پیراکهکشانی   
madim-e pirâkahkešâni

Fr.: milieu circumgalactique   

The interface between a galaxy and the → intergalactic medium. The circumgalactic medium comprises gas located in the → halo of a galaxy extending out to the → virial radius.

circum-; → galactic.

diffuse galactic light
  نور ِ کهکشانی ِ پخشیده   
nur-e kahkašâni-ye paxšidé

Fr.: lumière galactique diffuse   

A minor component of galactic light resulting from the diffusion of starlight by → interstellar dust near the → galactic plane.

diffuse; → galactic; → light.

extragalactic
  استرکهکشانی، برون‌کهکشانی   
ostar-kahkašâni, borun-kahkašâni

Fr.: extragalactique   

Of, pertaining to, or dealing with the space beyond the Milky Way.

From → extra- + → galactic.

extragalactic astronomy
  اخترشناسی ِ استرکهکشانی، ~ برون‌کهکشانی   
axtaršenâi-ye ostar-kahkašâni, ~ borun-kahkašâni

Fr.: astronomie extragalactique   

The branch of astronomy that deals with objects beyond the Milky Way, especially galaxies and quasars.

extragalactic; → astronomy.

extragalactic background light (EBL)
  نور ِ پس-زمینه‌ی ِ استر-کهکشانی   
nur-e paszimine-ye ostarkahkeši

Fr.: lumière du fond extragalactique   

The integrated intensity of all of the light emitted throughout the history of the Universe across the whole of the → electromagnetic spectrum, including those which are not individually detected. The EBL spectrum includes cosmological backgrounds associated with either primordial phenomena, such as the → cosmic microwave background radiation (CMBR), or photons emitted by stars, galaxies and → active galactic nuclei (AGN) due to → nucleosynthesis or other → radiative processes, including → dust scattering, → absorption and reradiation. The EBL may also contain signals that are diffuse and extended, including high-energy photons associated with dark matter particle decays or annihilation.

extragalactic; → background; → light.

galactic
  کهکشانی   
kahkešâni (#)

Fr.: galactique   

1) Of or pertaining to a → galaxy.
2) Usually with capital G, pertaining to our galaxy, the → Milky Way.

Adjective of → galaxy.

Galactic anticenter
  پادمرکز ِ کهکشان   
pâdmarkaz-e kahkešân

Fr.: anticentre galactique   

The point in the → Galactic plane that lies directly opposite the → Galactic center. It lies in the constellation → Auriga at approximately R.A. 05h 46m, Dec. +28° 56'.

galactic; → anticenter.

galactic bar
  میله‌ی ِ کهکشانی   
mile-ye kahkešâni

Fr.: barre galactique   

An elongated bar-shaped structure composed of stars present in some spiral galaxies. About two-third of such galaxies contain bars that cross their centers. Bars, like → spiral arms, result from a → density wave in which stars take very elliptical orbits. They form when the → galactic disk dominates the → galactic bulge, → Ostriker-Peebles criterion. Bars play an extremely important role in a galaxy's evolution. The gravity from a bar is the mechanism that drives → interstellar gas from the outer parts of a → spiral galaxy inward toward the central regions, and into the galactic nucleus itself. This causes tremendous bursts of star formation. Therefore, a majority of massive stars are born in such starbursts in the nuclei of galaxies. Bars may also channel the material that falls into black holes within active galactic nuclei, releasing enormous power in radiation and particles from tiny regions at the centers of some galaxies. Bars disappear as galactic centers grow more massive (after some 2 to 8 Gyr).

galactic; → bar.

Galactic bulge
  کوژ ِ کهکشان   
kuž-e kakhašân

Fr.: bulbe de la Galaxie   

The central → galaxy bulge of the → Milky Way.

galactic; → bulge.

Galactic Center
  مرکز ِ کهکشان   
markaz-e kahkešân (#)

Fr.: centre galactique   

1) The rotational center of the → Milky Way galaxy located in the direction of the → Sagittarius constellation at a distance of 7.62 ± 0.32 kpc (2005, ApJ 628, 246). Its equatorial coordinates (J2000 epoch) are: R.A. 17h45m40.04s, Dec. -29° 00' 28.1''. The Sun orbits around the Galactic center once every 200 million years at a speed of 220 km per second. It is believed that there is a → supermassive black hole at the Galactic center.
2) The innermost region of a → spiral galaxy characterized by high number of stars per unit volume. The center may contain a → supermassive black hole.

galactic; → center.

Galactic center cluster
  خوشه‌ی ِ مرکز ِ کهکشان   
xuše-ye markaz-e kahkešân

Fr.: amas du centre galactique   

One of the three massive clusters located toward the → Galactic center: → Quintuplet cluster, → Arches cluster, → Central cluster. Heavily extinguished by the presence of dust clouds and only accessible at infrared (and longer) wavelengths or in X-rays, each of these clusters has a population of more than a hundred → massive stars. The three clusters are similar in most respects, each containing about 104 solar masses in stars. The Arches cluster is younger than the two others.

galactic; → center; → cluster.

galactic cluster
  خوشه‌ی ِ کهکشانی، ~ کهکشانها   
xuše-ye kahkešâni, ~ kahkešânhâ

Fr.: amas galactique   

1) Same as → open cluster.
2) same as → cluster of galaxies.

galactic; → cluster.

Galactic coordinates
  هماراهای ِ کهکشانی   
hamârâhâ-ye kahkešâni

Fr.: coordonnées galactiques   

A system of astronomical coordinates using → latitude (bII) measured north and south from the → Galactic equator and → longitude (lII), measured from the → Galactic Center in the sense of increasing → right ascension from 0 to 360 degrees. In the old system (lI,bI), the Galactic center was at lI = 327°41'. Same as → galactic system.

galactic; → coordinate.

galactic disk
  گرده‌ی ِ کهکشان   
gerde-ye kahkešân

Fr.: disque galactique   

The flattened component of a → spiral galaxy which is composed of stars and concentrations of dust and molecules. → Star formation takes place mainly in the disk.

galactic; → disk.

galactic dynamics
  دینامیک ِ کهکشانی   
tavânik-e kakhešâni

Fr.: dynamique galactique   

The study of the → motions of the → stars, → gas, and → dark matter in a → galaxy to explain the main → morphological and → kinematical features of the galaxy.

galactic; → dynamics.

Galactic equator
  هموگار ِ کهکشان   
hamugâr-e kahkešân

Fr.: équateur galactique   

The great circle in the sky defined by the place of the → Galactic plane or the → Milky Way. At an angle of about 62°, the Galactic equator intersects the celestial equator at two points located in the constellations → Monoceros and → Aquila.

galactic; → equator.

Galactic habitable zone
  زنار ِ زیست‌پذیر ِ کهکشان   
zonâr-e zistpazir-e kahkešân

Fr.: zone habitable galactique   

A region of the Galaxy whose boundaries are set by its calm and safe environment and access to the chemical materials necessary for building terrestrial planets similar to the Earth. → circumstellar habitable zone; → habitable zone.

galactic, → habitable; → zone.

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