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HST Study of the Proper Motion of HST-1 in the Jet of M87

The radio galaxy M87 is well known for its jet, which features a series of bright knots observable from radio to X-ray wavelengths. The most famous of these, HST-1, exhibits superluminal motion, and our analysis of Chandra data reveals a correlation between the X-ray flux of HST-1 and its separation...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Egile Nagusiak: Rameshan Thimmappa, Joey Neilsen, Daryl Haggard, Mike Nowak, Łukasz Stawarz
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2026-01-01
Saila:The Astrophysical Journal
Gaiak:
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ae3e84
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