
NGC 1409 - Wikipedia
NGC 1409 is a quiescent [4] lenticular galaxy in the equatorial constellation of Taurus. It was discovered by the German-born astronomer William Herschel on January 6, 1785. [6] NGC 1409 is located in close proximity to the smaller Seyfert …
APOD: 2001 January 12 - NGC 1410/1409: Intergalactic Pipeline
NGC 1410/1409: Intergalactic Pipeline Credits: William C. Keel (Univ. Alabama, Tuscaloosa), NASA. Explanation: These two galaxies are interacting in a surprising way, connected by a "pipeline" of obscuring material that runs between them over 20,000 light-years of …
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Intergalactic 'Pipeline' Funnels Matter Between Colliding Galaxies NGC …
2001年1月9日 · Scientists believe that the tussle between these compact galaxies somehow created the pipeline, but they're not certain why NGC 1409 was the one to begin gravitationally siphoning material from its partner.
A Pipeline Found Between Two Galaxies | Scientific American
2001年1月10日 · Two galaxies in the constellation Taurus have locked horns: NGC 1409 and NGC 1410, bound by gravity, are spinning around each other at 670,000 miles an hour. And as this image taken by the...
Intergalactic 'Pipeline' Funnels Matter Between Colliding Galaxies NGC ...
The arms of NGC 1410, an active, gas-rich spiral galaxy classified as a Seyfert, are awash in blue, the signature color of star-forming regions. The bar of material bisecting the center of NGC 1409 also is a typical byproduct of galaxy collisions. Astronomers expect more fireworks to come.
NGC 1409 - Wikiwand
NGC 1409 is a quiescent lenticular galaxy in the equatorial constellation of Taurus. It was discovered by the German-born astronomer William Herschel on January...
NGC 1409 - 百度百科
NGC 1409 是金牛座的一个星系,星等为13.7。
NGC1409 & NGC1410 - Stellar Scenes
This image shows you a extraordinary faint colliding galactic pair positioned above a border of Taurus and Eridanus. The pair is estimated about 300 millions light years away, both galaxies has an apparent sizes of 1 arc minutes or so and 14th or 15th magnitude in visual brightness.
NGC 1409 – Wikipedia
NGC 1409 ist eine Spiralgalaxie vom Hubble-Typ SAB im Sternbild Stier, die 345 Millionen Lichtjahre von der Milchstraße entfernt ist. Sie befindet sich in Wechselwirkung mit der Galaxie NGC 1410, von der sie rund 23.000 Lichtjahre entfernt ist.
- 某些结果已被删除