Probing extreme black-hole outflows on short timescales via high spectral-resolution x-ray imagers
Document Type
Article
Publication Date
7-1-2024
Publication Title
Astronomische Nachrichten
Abstract
We investigate outflows and the physics of super-Eddington versus sub-Eddington regimes in black hole systems. Our focus is on prospective science using next-generation high-resolution soft x-ray instruments. We highlight the properties of black hole ultraluminous x-ray source (ULX) systems in particular. Owing to scale invariance in accreting black holes, ULX accretion properties, including their outflows, inform our understanding not only of the closely related population of (similar-mass) x-ray binary systems but also of tidal disruption events (TDEs) around supermassive black holes. A subsample of TDEs are likely to transcend super-Eddington to sub-Eddington regimes as they evolve, offering an important unifying analog to ULXs and sub-Eddington x-ray binaries. We demonstrate how next-generation soft x-ray observations with resolving power (Formula presented.) and collecting area (Formula presented.) can simultaneously identify ultrafast and more typical wind components, distinguish between different wind mechanisms, and constrain changing wind properties over characteristic variability timescales.
Volume Number
345
Issue Number
6-7
DOI
10.1002/asna.20240027
Recommended Citation
Pinto, C.; Steiner, J. F.; Bodaghee, A.; Chakraborty, P.; Sobolewska, M.; Pasham, D. R.; Ogorzalek, A.; Zuhone, J.; Bogdan, A.; and Vogelsberger, M., "Probing extreme black-hole outflows on short timescales via high spectral-resolution x-ray imagers" (2024). Faculty and Staff Works. 1010.
https://kb.gcsu.edu/fac-staff/1010