
NGC 740 - Wikipedia
NGC 740 is a barred spiral galaxy located in the Triangulum constellation. It is estimated to be 210 million light-years from the Milky Way and has a diameter of about 85,000 light-years. It was discovered by the Irish engineer Bindon Stoney , an assistant to William Parsons .
NGC 740 - 维基百科,自由的百科全书
ngc 740 是三角座的一個星系。 维基共享资源上的相關多媒體資源:ngc 740. ned – ngc 740; seds – ngc 740; simbad – ngc 740; vizier – ngc 740
NGC 740 - Barred Spiral Galaxy in Triangulum | TheSkyLive.com
NGC 740 is a Barred Spiral Galaxy in the Triangulum constellation. NGC 740 is situated north of the celestial equator and, as such, it is more easily visible from the northern hemisphere. Given its B magnitude of 14.9, NGC 740 is visible with the help of a telescope having an aperture of 20 inches (500mm) or more.
NGC 740 - Simple English Wikipedia, the free encyclopedia
NGC 740 is a barred spiral galaxy in the Triangulum constellation. It is about 212 million light-years away from the Milky Way.
NGC 740 - 百度百科
NGC 740 是三角座的一个星系,1850年10月11日被威廉·帕森思发现。
NGC 740 - Wikiwand
NGC 740 is a barred spiral galaxy located in the Triangulum constellation. It is estimated to be 210 million light-years from the Milky Way and has a diameter of about 85,000 light-years. It was discovered by the Irish engineer Bindon Stoney , an assistant to William Parsons .
NGC 740 - 维基百科,自由的百科全书 - zh.wikipedia.org
NGC 740 是 三角座 的一个 星系。 维基共享资源 上的相关多媒体资源: NGC 740.
NGC 740 | galaxy in Triangulum | NGC List | GO ASTRONOMY
NGC 740 . NGC 740 is a barred spiral galaxy located in the constellation Triangulum. Some key stats include:
NGC 740 Galaxy Facts (UGC 1421) - Universe Guide
2024年1月1日 · NGC 740 is a Spiral Galaxy located in the constellation of Triangulum in the northern hemisphere. NGC 740's distance from Earth is 209,320,640.08 light years. NGC 740 is called NGC 740 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.
NGC 740 - 银河 - SKY-MAP
Molecular gas in the galaxy cluster Abell 262. CO observations of UGC 1347 and other galaxies of the cluster We present millimeter CO line emission observations of 12 galaxieswithin the Abell 262 cluster, together with L_FIRdata, in the context of a possible molecular gas deficiency within theregion of the cluster center.
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