Übersetzung für 'disc galaxy' von Englisch nach Deutsch

disc galaxy

Scheibengalaxie {f}astron.

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magneto-optical disc <MOD, MO disc>

magnetooptische Diskette {f} <MOD, MO-Disk, MO-Diskette>comp.

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galaxy

Sternsystem {n}astron.

Galaxie {f}astron.

double galaxy

Doppelgalaxie {f}astron.

host galaxy

Heimatgalaxie {f}astron.

radio galaxy

Radiogalaxie {f}astron.

ring galaxy

Ringgalaxie {f}astron.

galaxy formation

Galaxienbildung {f}astron.

Galaxienentstehung {f}astron.

parent galaxy

Muttergalaxie {f}astron.

Triangulum Galaxy

Dreiecksnebel {m}astron.

galaxy encounter

Begegnung {f} von Galaxienastron.

starburst galaxy

Starburstgalaxie {f}astron.

dark galaxy

dunkle Galaxie {f} [auch Dunkle Galaxie]astron.

lenticular galaxy

lentikuläre Galaxie {f}astron.

Linsengalaxie {f}astron.

galaxy collision

Galaxienkollision {f}astron.

disk galaxy

Scheibengalaxie {f}astron.

Seyfert galaxy

Seyfertgalaxie {f}astron.

galaxy evolution

Galaxienentwicklung {f}astron.

• The disc galaxy DLA0817g is nicknamed the Wolfe Disc in his honor.
• A likely outcome of the collision is that the galaxies will merge to form a giant elliptical galaxy or possibly large disc galaxy.
• A disc galaxy (or disk galaxy) is a galaxy characterized by a galactic disc, a flattened circular volume of stars.
• They explored tight correlations that exist between supermassive black hole masses and large-scale properties of the host galaxy, as well as described how halo properties determine those of a disc galaxy and its supermassive black hole.
• It is a large rotating disc galaxy, with a mass of approximately 72 billion solar masses, dating back to an early age in the life of the universe, approximately 1.5 billion years after the Big Bang.

• NGC 6670E (also known as NGC 6670-1 and NGC 6670B) is a disc galaxy on the north-eastern side of NGC 6670.
• Lindblad resonances affect stars at such distances from a disc galaxy's centre where the natural frequency of the radial component of a star's orbital velocity is close to the frequency of the gravitational potential maxima encountered during its course through the spiral arms.