NGC 7319 is a highly distorted barred spiral galaxy that is a member of the compact Stephan's Quintet [5] group located in the constellation Pegasus, some 311 megalight-years distant from the Milky Way. [1] It was discovered on 27 September 1873 by French astronomer Édouard Stephan. [6]

ngc 7319是位於飛馬座的一個棒渦星系，與ngc 7317、ngc 7318a、ngc 7318b、和ngc 7320c共同組成史蒂芬五重星系。

拍摄您当地的文化，帮助维基百科并赢得比赛！ NGC 7319 是位于 飞马座 的一个 棒涡星系，与 NGC 7317 、 NGC 7318a 、 NGC 7318b 、和 NGC 7320c 共同组成 史蒂芬五重星系。 ^ 1.0 …

NGC 7319 NIRCAM plus MIRI Stephan's Quintet This grouping of galaxies is located in the constellation Pegasus, about 280 million light-years from the Solar System. It was the first such compact group discovered and is also called Hickson Compact Group 92. 4 galaxies are physically connected and interacting: NGC 7318 A and B, NGC7319, and ...

2023年7月25日 · NGC 7319, at top right, is a barred spiral with distinct spiral arms that extend from the ends of the bar. The blue specks in the spiral arm at the top of NGC 7319 and the red dots just above and to the right of the core are clusters of many thousands of stars.

2022年8月9日 · NGC7319 hosts a type 2 active galactic nucleus (AGN) and a low-power radio jet (L_1.4GHz=3.3x10^22 W Hz^-1) with two asymmetric radio hotspots at 430 pc (N2) and 1.5 kpc (S2) projected distances from the unresolved radio core.

NGC 7319 is a Spiral Galaxy in the Pegasus constellation. NGC 7319 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its visual magnitude of 13.53, NGC 7319 is visible with the help of a telescope having an aperture of 14 inches (350mm) or more.

It was the first such compact group discovered and is also called Hickson Compact Group 92. 4 galaxies are physically connected and interacting: NGC 7318 A and B, NGC7319, and NGC7317 (and possibly NGC7320c).

NGC 7319是位于 飞马座 的一个棒涡星系，与 NGC 7317 、NGC 7318a、NGC 7318b、和 NGC 7320c 共同组成史蒂芬五重奏。 史蒂芬五重星系是由五个可见光的星系组成的集团，其中四个组成被发现的第一个 致密星系团。 这个集团是爱德华·史提芬在1877年于马赛天文台发现的。 这个集团是所有的致密星系团中被研究得最多的，集团中可见的最亮成员是 螺旋星系 NGC 7320 显示出有广大的 电离氢区，以红色的小滴辨识，有活跃的恒星形成活动。 NGC 7319是位于飞马座的 …

The photo showcases three regions of star birth: the long, sweeping tail and spiral arms of the galaxy NGC 7319 (near center); the gaseous debris of two galaxies, NGC 7318B and NGC 7318A (top right); and the area north of those galaxies, dubbed the northern starburst region (top left).