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  1. NGC 128 - Wikipedia

    NGC 128 is a lenticular galaxy in the constellation Pisces. It is approximately 190 million light-years from the Sun and has a diameter of about 165,000 light-years. [2] NGC 128 was discovered by astronomer William Herschel on 25 December 1790 using a reflecting telescope with an aperture of 18.7 inches.

  2. NGC 128 Group in Pisces - Webb Deep-Sky

    The LGG 6 group is composed of 11 galaxies including NGC 128, NGC 126, NGC 127 and NGC 130. Nearby MCG +0-2-45 is also associated with the group. NGC 128 itself appears to be interacting with NGC 127 and there is a tidal tail between the two.

  3. Observing at Skyhound: NGC 128

    NGC 128 is a tiny edge-on spiral galaxy distorted by tidal interaction with one or more neighboring galaxies. Walter Scott Houston wrote that he was able to view this galaxy in his 5-inch from a dark site. An 8-10 inch instrument will show the peculiar box-shape at the center.

  4. NGC 128 - Lenticular Galaxy in Pisces | TheSkyLive.com

    NGC 128 is a Lenticular Galaxy in the Pisces constellation. NGC 128 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year.

  5. Astronomers detect double ‘peanut shell’ galaxies

    May 8, 2016 · Using data from the NASA/ESA Hubble Space Telescope and the Sloan Digital Sky Survey, the researchers realised that two of the galaxies they were studying — NGC 128 and NGC 2549 — were quite exceptional.

  6. NGC 128 - Deep Sky Observing - Cloudy Nights

    Sep 3, 2024 · As I am going through Don Pensak's best of 500 list, I came across NGC 128 at mag 11.6. Since it's not even in the Pocket Sky Atlas, I had my doubts, but I've come to realize that on this list there are distant open clusters that at 343x on my Obsession 18" look pretty fantastic, so I persist.

  7. Title: Structure and kinematics of the peculiar galaxy NGC 128

    Sep 16, 1998 · This is a multiband photometric and spectroscopic study of the peculiar S0 galaxy NGC128. We present results from broad (B and R) and narrow band optical CCD photometry, near (NIR) and far (FIR) infrared observations, long slit spectroscopy, and Fabry-Perot interferometry (CIGALE).

  8. The NGC 128 Group of Galaxies - SpringerLink

    I present preliminary results of a 2D photometric and kinematic study of the NGC 128 group of galaxies (NGC 127, NGC 128 and NGC 130). There is strong evidence that these three galaxies are currently suffering a strong dynamical interaction.

  9. NGC 128 - 维基百科,自由的百科全书

    NGC 128 (UGC 292, MCG 0-2-51, ZWG 383.29, PGC 1791)是 雙魚座 的一個 星系。 星等 為11.8, 赤經 為29分14.9秒, 赤緯 為2°51'54"。 在1790年12月25日被 弗里德里希·威廉·赫歇爾 …

  10. NGC 128 Galaxy Group - AstroBin

    This object is a rarely imaged galaxy cluster located 190 million light years away in the constellation of Pisces at a declination of +3 degrees. The cluster is anchored by NGC 128, a lenticular ga...

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