Type-C QPOs in MAXI J1348-630 exhibit stable ~7 Hz frequency despite intensity changes, hard rms spectra with peaks above 20 keV, and opposite hysteresis in frequency-flux relations between main and mini-outbursts.
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New optical identifications and precise astrometry are reported for four quiescent black hole X-ray transients, with 3-sigma magnitude limits for five additional candidates.
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The full evolution of the type-C QPO in MAXI J1348-630 revealed by Insight-HXMT
Type-C QPOs in MAXI J1348-630 exhibit stable ~7 Hz frequency despite intensity changes, hard rms spectra with peaks above 20 keV, and opposite hysteresis in frequency-flux relations between main and mini-outbursts.
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A search for optical counterparts in quiescent black hole X-ray transients
New optical identifications and precise astrometry are reported for four quiescent black hole X-ray transients, with 3-sigma magnitude limits for five additional candidates.