
3C 75 - Wikipedia
3C 75 (also called 3C75) is a binary black hole system in the dumbbell-shaped galaxy NGC 1128 in the galaxy cluster Abell 400. It has four relativistic jets, two coming from each accreting supermassive black hole.
3C 75 - 维基百科,自由的百科全书
3C 75 是位於 阿貝爾 400 星系團 中啞鈴形星系 NGC 1128 一個雙 黑洞 系統,有四個 相對論 性噴流,其中兩個來自 超大質量黑洞。 噴流以每秒1,200 公里 的速度移動。 3C 75可能是X射線源2A 0252+060(1H 0253+058、XRS 02522+060) [4]。 ^ SIMBAD. [2023-09-30]. (原始内容 存档 于2015-05-25). ^ 跳转到: 2.0 2.1 NASA/IPAC Extragalactic Database. Results for 3C 75. [2010-04-26]. ^ Nemiroff, R.; Bonnell, J. (编). Two Black Holes Dancing in 3C 75.
3C 75里的旋舞双黑洞 | NASA中文
Jun 5, 2022 · The two bright sources at the center of this composite x-ray (blue)/ radio (pink) image are co-orbiting supermassive black holes powering the giant radio source 3C 75. Surrounded by multimillion degree x-ray emitting gas, and blasting out jets of relativistic particles the supermassive black holes are separated by 25,000 light-years.
APOD: 2010 March 14 - Binary Black Hole in 3C 75
There, two bright sources at the center of this composite x-ray (blue)/radio (pink) image are thought to be co-orbiting supermassive black holes powering the giant radio source 3C 75. Surrounded by multimillion degree x-ray emitting gas, and blasting out jets of relativistic particles the supermassive black holes are separated by 25,000 light ...
APOD: 2017 October 22 - Two Black Holes Dancing in 3C 75
The two bright sources at the center of this composite x-ray (blue)/ radio (pink) image are co-orbiting supermassive black holes powering the giant radio source 3C 75. Surrounded by multimillion degree x-ray emitting gas, and blasting out jets of relativistic particles the supermassive black holes are separated by 25,000 light-years.
3C 75 - Wikiwand
3C 75 (also called 3C75) is a binary black hole system in the dumbbell-shaped galaxy NGC 1128 in the galaxy cluster Abell 400. It has four relativistic jets, two coming from each accreting supermassive black hole.
在3C 75内旋舞的双黑洞 - 新浪财经网
Oct 2, 2023 · 活跃星系3c 75的核心发生什么事?这幅结合x射线(蓝)及电波波段(粉红)影像里的亮斑,是二颗相互旋绕的超大质量黑洞,它们也是庞大电波源3c 75的能量源。 这二个相距隔约25,000光年的超大质量黑洞,周围包围着温度高达数百万度的X射线辐射云气,并喷出相对论性的粒子 ...
3C 75
Data at NED - NASA/IPAC Extragalactic Database : 3C 75. Link by name to the catalogue in VizieR:
Photo Album :: 3C 75 in Abell 400 - Chandra
These black holes are in the dumbbell galaxy NGC 1128, which has produced the giant radio source, 3C 75. This image from the Digitized Sky Survey (DSS)/Palomar 48-inch Schmidt telescope shows NGC 1128 in visible light. The peculiar dumbbell structure of this galaxy is thought to be due to two large galaxies that are in the process of merging.
3C 75 - 維基百科,自由的百科全書 - zh.wikipedia.org
3C 75 是位於 阿貝爾 400 星系團 中啞鈴形星系 NGC 1128 一個雙 黑洞 系統,有四個 相對論 性噴流,其中兩個來自 超大質量黑洞。 噴流以每秒1,200 公里 的速度移動。 3C 75可能是X射線源2A 0252+060(1H 0253+058、XRS 02522+060) [4]。 ^ SIMBAD. [2023-09-30]. (原始內容 存檔 於2015-05-25). ^ 移至: 2.0 2.1 NASA/IPAC Extragalactic Database. Results for 3C 75. [2010-04-26]. ^ Nemiroff, R.; Bonnell, J. (編). Two Black Holes Dancing in 3C 75.