Making the Invisible Visible: Magnetic Fields in Accretion Flows Revealed by X-Ray Polarization
Large-scale, strong magnetic fields are often evoked in black hole accretion flows, for jet launching in the low/hard state and to circumvent the thermal instability in the high/soft state. Here, we show how these ideas are strongly challenged by X-ray polarization measurements from the Imaging X-ra...
Saved in:
| Main Authors: | Samuel Barnier, Chris Done |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad9277 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
X-Ray Spectra of Black Hole X-Ray Binaries with Returning Radiation
by: Temurbek Mirzaev, et al.
Published: (2024-01-01) -
X-Ray Polarization Variability during a Few Hz Quasiperiodic Oscillations in Swift J1727.8-1613 Observed with IXPE
by: Kaito Ninoyu, et al.
Published: (2025-01-01) -
On the Broadening of the Characteristic Frequency Range toward Higher Photon Energies in the X-Ray Variability of the Black Hole Transient MAXI J1820+070
by: ChenXu Gao, et al.
Published: (2025-01-01) -
X-Ray and Optical Polarization Aligned with the Radio Jet Ejecta in GX 339–4
by: G. Mastroserio, et al.
Published: (2025-01-01) -
Simulation-based Prediction of Black Hole X-Ray Spectra and Spectral Variability
by: Rongrong Liu, et al.
Published: (2025-01-01)