Detecting Iron Line Profile Variability During Tearing Events in Stellar Mass Black Hole Accretion Disks with HEX-P

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (<10 arcsec FWHM) and broad spectral coverage (0.1-150 keV) with an effective area far superior to current facilities (including XMM-Newton and NuSTAR) to enable revolutionary new insights into a variety of important astrophysical problems.

More information on HEX-P, including the full team list, is available at https://hexp.org.