
NGC 4395 - Wikipedia
NGC 4395 is a nearby low surface brightness spiral galaxy located about 14 million light-years (or 4.3 Mpc) from Earth in the constellation Canes Venatici. [1] The nucleus of NGC 4395 is active …
Hubble Gazes at the Home of an Enormous Black Hole
2023年5月2日 · This NASA Hubble Space Telescope image of the spiral galaxy NGC 4395 looks at a small section of the larger galaxy. As galaxies go, NGC 4395 has a very low surface …
NGC 4395 - 维基百科,自由的百科全书
NGC 4395 是一個 低表面亮度 螺旋星系 有著直徑大約8&prime 的暈。 從它的西北到東南,有幾個較寬闊的區域有著較高的亮度,最亮的區域在最遠的東南方。
NGC 4395 - Spiral Galaxy in Canes Venatici - TheSkyLive.com
NGC 4395 is a Spiral Galaxy in the Canes Venatici constellation. NGC 4395 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. …
Ground-based image of Seyfert galaxy NGC 4395 - ESA/Hubble
1993年7月16日 · This photograph of the nearest Seyfert galaxy, NGC 4395, was taken with the Palomar 200-inch telescope. NGC 4395 is the least luminous and nearest Seyfert galaxy …
NGC 4395 - low surface brightness spiral in CVn - AstroBin
NGC 4395 is a nearby low surface brightness spiral galaxy located about 14 million light-years (or 4.3 Mpc) from Earth in the constellation Canes Venatici. The nucleus of NGC 4395 is active …
NGC 4395 Galaxy (UGC 7524) Facts & Distance - Universe Guide
NGC 4395 is a Seyfert 2 Galaxy located in the constellation of Canes Venatici in the northern hemisphere. NGC 4395's distance from Earth is 13,897,523.25 light years.
Spiral Galaxy NGC 4395 | NOIRLab
2020年6月30日 · NGC 4395 is a spiral galaxy with a very low surface brightness. Unlike most galaxies the center of the galaxy is small and faint. Nearly all galaxies are known to contain a …
Star Formation in the Dwarf Seyfert Galaxy NGC 4395 ... - IOPscience
2023年6月13日 · We present a detailed multiwavelength study of star formation in the dwarf galaxy NGC 4395, which hosts an active galactic nucleus (AGN). From our observations with …
Galaxy NGC 4395 - Deep⋆Sky Corner
NGC 4395 is a galaxy of the morphological type SAB, an intermediate form from a spiral to a barred spiral. It is a Seyfert 2 galaxy with a bright core but low surface brightness. The …
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