ausblenden:
Schlagwörter:
SAGITTARIUS-A-ASTERISK; PARSEC-SCALE JET; FERMI BUBBLES; RADIO LOBES;
MILKY-WAY; ORIGIN; ABSORPTION; OUTFLOW; ECHOES; VIEWAstronomy & Astrophysics;
Zusammenfassung:
Using deep archival observations from the Chandra X-ray Observatory, we present an analysis of linear X-ray-emitting features located within the southern portion of the Galactic center chimney and oriented orthogonal to the Galactic plane, centered at coordinates l = 0.degrees 08, b = -1.degrees 42. The surface brightness and hardness ratio patterns are suggestive of a cylindrical morphology, which may have been produced by a plasma outflow channel extending from the Galactic center. Our fits of the feature's spectra favor a complex two-component model consisting of thermal and recombining plasma components, possibly a sign of shock compression or heating of the interstellar medium by outflowing material. Assuming a recombining plasma scenario, we further estimate the cooling timescale of this plasma to be on the order of a few hundred to thousands of years, leading us to speculate that a sequence of accretion events onto the Galactic black hole may be a plausible quasi-continuous energy source to sustain the observed morphology.
