NGC 1566 - Wikipedia
NGC 1566 is an active galaxy with many features of a Seyfert type 1, although the exact type remains uncertain. It is one of the closest and brightest Seyfert galaxies. The mass of the supermassive black hole at the center is estimated at (1.3 ± 0.6) × 107 M☉.
NGC 1566 - 维基百科，自由的百科全书
ngc 1566 是剑鱼座的一個中間螺旋星系。由詹姆士·丹露帕發現於1826年5月28日。該星系是劍魚座星系團的重要成員星系 [3] ，並且是其中亮度最高者 [4] [5] 該星系是已知最明亮的塞弗特星系之一 [3] 。
Composite Image of NGC 1566 - NASA
2022年4月20日 · Composite Image of NGC 1566. This galaxy is part of a large survey of more than 100 galaxies conducted by Chandra that looked for evidence of growing black holes. A new study uncovered evidence that stellar-mass black holes in these dense environments are ripping apart multiple stars, and then using their debris to fuel their growth.
Hubble Tangos with a Dancer in Dorado - NASA Science
2023年11月3日 · This vibrant Hubble Space Telescope image features the spiral galaxy NGC 1566, sometimes informally referred to as the ‘Spanish Dancer Galaxy’. Like the subject of another recent image, NGC 1566 is a weakly-barred or intermediate spiral galaxy.
NGC 1566 - 百度百科
ngc 1566 是剑鱼座的一个中间螺旋星系。 由詹姆士·丹露帕发现于1826年5月28日。 该星系是剑鱼座星系团的重要成员星系，并且是其中亮度最高者该星系是已知最明亮的塞弗特星系之一。
APOD: 2019 July 2 - NGC 1566: The Spanish Dancer Spiral Galaxy
Classified as a grand design spiral, NGC 1566's shows two prominent and graceful spiral arms that are traced by bright blue star clusters and dark cosmic dust lanes. Numerous Hubble Space Telescope images of NGC 1566 have been taken to study star formation, supernovas, and the spiral's unusually active center
NGC 1566 - Science@NASA
ngc 1566 The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centers of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harboring supermassive black holes that are many millions of times the ...
Grand Swirls from NASA’s Hubble - Science@NASA
2014年6月6日 · This new Hubble image shows NGC 1566, a beautiful galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well-defined bar-shaped region of stars at its center — like barred spirals — it is not quite […]
NGC 1566: 韦伯与哈勃的螺旋星系影像 – NASA中文
2024年2月6日 · 几乎没有，也因此西班牙舞者星系（ngc 1566）是天空中最典型和最上镜头的螺旋星系之一。 不过， 这幅星系影像 倒是有一些特别之处，因为它是两张照片以对角线并接：左上角的来自 哈勃太空望远镜 ，右下角的则是 韦伯太空望远镜 的照片。
Webb and Hubble's Views of Spiral Galaxy NGC 1566
2024年1月29日 · Hubble’s image of NGC 1566 shows a densely populated face-on spiral galaxy anchored by its central region, consisting of a core and small bar structure, which has a light yellow haze of stars that takes up about a quarter of the view. The core is brightest at the center, washing out some light from other objects.
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