
SS 433 - Wikipedia
SS 433 is a microquasar or eclipsing X-ray binary system, consisting of a stellar-mass black hole accreting matter from an A-type companion star. [5] [6] SS 433 is the first discovered microquasar. [7] It is at the centre of the supernova remnant W50.
SS 433 - 百度百科
ss 433(ss433)是一个食双星系统,其主星可能是一个黑洞,或中子星。同时是第一个被发现具有喷流的x射线双星。它位于超新星遗迹w50中心,估计年龄大约10000年左右。ss 433附近有伴星作轨道运动并为吸积盘提供物质。
Very-high-energy particle acceleration powered by the jets of the ...
Oct 3, 2018 · SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star)1–3.
Very high energy particle acceleration powered by the jets of …
Oct 3, 2018 · Abstract: SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star). Two jets of ionized matter with a bulk velocity of $\sim0.26c$ extend from the binary, perpendicular to the line of sight, and terminate inside W50, a supernova ...
SS 433 - 维基百科,自由的百科全书
ss 433是觀測到的最奇特恆星系統之一。 它位於 銀河系 ,並且是一個 食雙星 、 X射線聯星 的 系統 ,主星是恆星質量的 黑洞 [ 5 ] , 伴星 的光譜表明它是一顆晚期的 A型星 [ 7 ] 。
APOD: 2020 August 31 - SS 433: Binary Star Micro Quasar
SS 433: Binary Star Micro-Quasar Animation Credit: DESY, Science Communication Lab. Explanation: SS 433 is one of the most exotic star systems known. Its unremarkable name stems from its inclusion in a catalog of Milky Way stars which emit radiation characteristic of …
Chandra :: Photo Album :: SS 433 :: January 17, 2024
Microquasar SS 433 sits in the center of the supernova remnant W50 in the constellation Aquila, some 18,000 light-years from Earth. SS 433’s powerful jets, which distort the remnant’s shape and earned it the nickname the “Manatee Nebula,” have been clocked at roughly 26% of the speed of light, or more than 48,000 miles per second.
Gamma-ray heartbeat powered by the microquasar SS 433
Aug 17, 2020 · Nature Astronomy - Ten years of gamma-ray data reveal emission in the vicinity of the microquasar SS 433 that is co-spatial with an interstellar gas enhancement and varies periodically at the...
SS 433 - Astronomy Magazine
Jan 1, 2024 · SS 433 consists of an A-type star orbiting a stellar-mass black hole surrounded by an accretion disk. Powerful X-rays radiate energy away from the disk as opposing jets of superheated gas shoot...
SS 433:双星系统形成的微类星体 | NASA中文
Sep 1, 2020 · Because the disk and jets from SS 433 resemble those surrounding supermassive black holes in the centers of distant galaxies, SS 433 is considered a micro-quasar. As illustrated in the animated featured video based on observational data, a massive, hot, normal star is locked in orbit with the compact object.