NGC 1760 是位於 剑鱼座 的一個 發射星雲。 該星雲位於 大麦哲伦星系,位于NGC 1761西南。 有9-10颗恒星與它有關。 NGC 1743於 1826年 由 蘇格蘭 的 詹姆士·敦洛普 發現。 [1] ^ Harold G. Corwin, Jr. Notes on the NGC objects, particularly those missing, misidentified, or otherwise unusual (ngcnotes.all). [2021-02-04]. （原始内容 存档 于2018-01-30） （英语）. 维基共享资源 上的相關多媒體資源： NGC 1760.

NGC 1760 是位於 劍魚座 的一個 發射星雲。 該星雲位於 大麥哲倫星系,位於NGC 1761西南。 有9-10顆恆星與它有關。 NGC 1743於 1826年 由 蘇格蘭 的 詹姆士·敦洛普 發現。 [1] ^ Harold …

NGC 1760 (also designated LHA 120-N 11, informally N11) is an emission nebula, or actually a complex ring of emission nebulae connected by glowing filaments over 1000 light-years across and located about 160,000 light-years away within the Large Magellanic Cloud, in the constellation of Dorado.

NGC 1760, also known as LHA 120-N 11 or simply N11, is a complex emission nebula spanning over 1,000 light-years. It is one of the most active star-forming regions in the nearby Universe and the second-largest in the LMC, surpassed only by the Tarantula Nebula

NGC 1760 (also known as Henize 11 or N 11) is star-forming region in the Large Magellanic Cloud (LMC) – a satellite galaxy to our Milky Way about 163,000 light-years away from Earth. This is the second largest of such in the LMC after NGC 2070 (Tarantula Nebula). It is a cocoon shaped nebula that consists of different components.

Description: This composite image features NGC 1760 and NGC 1747, two distinct regions within the Large Magellanic Cloud (LMC), located approximately 160,000 light-years away in the constellation of ...

NGC 1760, Nebula in the Large Magellanic Cloud One of the largest nebulas yet detected is actually a complex ring of emission nebulas connected by glowing filaments. The unusual network, known as N11, spans over 1000 light years, 160,000 light years away, and is a prominent structure of the Large Magellanic Cloud, the largest satellite galaxy ...

NGC 1760 is an star-forming complex nebula in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way. The overall complex of glowing gas and stars is known as N11 while the central cluster of hot young blue stars is know as NGC 1760.

2022年11月11日 · The brightest nebula in the LMC, sometimes referred to as The Bean Nebula, NGC 1760 is a star forming area with a very impressive emission nebula. It is located around 160,000 light years away in the Large Magellanic Cloud. Imaged in SHO narrowband with RGB stars on our RiDK 400 at Observatorio El Sauce, Chile. Image Processing: Mike Selby.

NGC 1760 is the brightest emission nebula of the Large Magellanic Cloud in the constellation of Dorado.NGC 1760 complex is the second-largest emission nebula (the largest is the Tarantula Nebula) cove...