NGC 326 is a dumbbell galaxy in the constellation Pisces. It was discovered on August 24, 1865 by Heinrich d'Arrest. It was described by Dreyer as "faint, a little extended, 9th or 10th magnitude star to southeast." [2]

NGC 326 是 雙魚座 的一個 星系。

NGC 326 is a Galaxy Pair in the Pisces constellation. NGC 326 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. The image below is a photograph of NGC 326 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the ...

Dec 12, 2011 · Abstract: NGC 326 is one of the most prominent X- or Z-shaped radio galaxies (XRGs/ZRGs) and has been the subject of several studies attempting to explain its morphology through either fluid motions or reorientation of the jet axis. We examine a 100 ks archival Chandra exposure and find several features associated with the radio galaxy: a high ...

We present new 144-MHz Low-Frequency Array (LOFAR) observations of the prototypical `X-shaped' radio galaxy NGC 326, which show that the formerly known wings of the radio lobes extend smoothly into a large-scale, complex radio structure.

Feb 6, 2012 · NGC 326 is one of the most prominent X-shaped galaxies and has been the subject of several studies attempting to find an explanation of its morphology through fluid motion or a reorientation of the jet axis. The study used the Chandra X-ray Observatory to examine the emissions of the radio galaxy.

Jul 11, 2019 · We present new 144-MHz Low-Frequency Array (LOFAR) observations of the prototypical ‘X-shaped’ radio galaxy NGC 326, which show that the formerly known wings of the radio lobes extend smoothly into a large-scale, complex radio structure.

Feb 20, 2012 · NGC 326 is one of the most prominent 'X'- or 'Z'-shaped radio galaxies (XRGs/ZRGs) and has been the subject of several studies attempting to explain its morphology through either fluid motions or reorientation of the jet axis.

We present new 144-MHz LOFAR observations of the prototypical `X-shaped' radio galaxy NGC 326, which show that the formerly known wings of the radio lobes extend smoothly into a large-scale, complex radio structure. We argue that this structure is most likely the result of hydrodynamical effects in an ongoing group or cluster merger, for which pre-existing X-ray and optical data provide ...

NGC 326 是 双鱼座 的一个 星系。 维基共享资源 上的相关多媒体资源： NGC 326.