
NGC 3628 - Wikipedia
NGC 3628, also known as the Hamburger Galaxy[3] or Sarah's Galaxy, [4][5][6][7][8] is an unbarred spiral galaxy about 35 million light-years away in the constellation Leo. It was discovered by William Herschel in 1784. It has an approximately 300,000 light-years long tidal tail.
NGC 3628: Hamburger Galaxy - Messier Objects
Jul 2, 2015 · NGC 3628, also known as the Hamburger Galaxy or Sarah’s Galaxy, is a famous unbarred spiral galaxy located in Leo constellation. The galaxy is about 100,000 light years across and occupies an area of 15 by 3.6 arcminutes of the apparent sky.
NGC 3628 - Barred Spiral Galaxy in Leo | TheSkyLive.com
NGC 3628 is a Barred Spiral Galaxy in the Leo constellation. NGC 3628 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.
APOD: 2020 June 4 - Portrait of NGC 3628
Explanation: Sharp telescopic views of NGC 3628 show a puffy galactic disk divided by dark dust lanes. Of course, this deep portrait of the magnificent, edge-on spiral galaxy puts some astronomers in mind of its popular moniker, the Hamburger Galaxy.
APOD: 2005 April 8 - Sideways Galaxy NGC 3628
Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. Explanation: Dark dust lanes cutting across the middle of this gorgeous island universe strongly hint that NGC 3628 is …
APOD: 2018 September 5 - NGC 3628: Sideways Spiral Galaxy
Featured is a sharp telescopic view of a magnificent edge-on spiral galaxy NGC 3628, a puffy galactic disk divided by dark dust lanes. Of course, this deep galactic portrait puts some astronomers in mind of its popular moniker, The Hamburger Galaxy.
The Core Starbursts of the Galaxy NGC 3628: Radio Very Long ...
Jul 14, 2023 · This work presents VLBI 1.5 GHz observational studies of the starburst galaxy NGC 3628, and this observation aimed to search for the potential low-luminosity AGN in NGC 3628, probe the nuclear radio sources, and constrain their sizes.