A bright flare in GRS 1915+105's obscured state arises from enhanced intrinsic emission plus reduced obscuration, with stratified absorber-reflector geometry consistent with re-illumination after a failed disk wind and a delayed radio flare.
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A bright flare in the obscured state of GRS 1915+105 as seen by NICER and Swift
A bright flare in GRS 1915+105's obscured state arises from enhanced intrinsic emission plus reduced obscuration, with stratified absorber-reflector geometry consistent with re-illumination after a failed disk wind and a delayed radio flare.