A sudden increase in the rate at which material reaches the most internal part of an accretion disk, i.e., the boundary layer, can change its structure dramatically. We have witnessed such a change for the first time in the symbiotic recurrent nova T CrB. Our analysis of XMM-Newton, Swift Burst Alert Telescope (BAT)/X-Ray Telescope (XRT)/UltraViolet Optical Telescope (UVOT), and the American Association of Variable Stars Observers (AAVSO) V- and B-band data indicates that during an optical brightening event that started in early 2014 (ΔV ≈ 1.5) the following occurred: (i) the hard X-ray emission as seen with BAT almost vanished; (ii) the XRT X-ray flux decreased significantly, while the optical flux remained high; (iii) the UV flux increase...
RS Ophiuchi is a recurrent nova system that experiences outbursts every ~20 years, implying accretio...
1ES 1927+654 is a paradigm-defying AGN and one of the most peculiar X-ray nuclear transients. In ear...
Nova LMC 2009a is confirmed as a Recurrent Nova (RN) from positional coincidence with nova LMC 1971b...
A sudden increase in the rate at which material reaches the most internal part of an accretion disk,...
The current superactive state of the recurrent nova T Coronae Borealis (T CrB) has been observed wit...
Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries in...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Estimates of the accretion rate in symbiotic recurrent novae (RNe) often fall short of theoretical e...
The tenth recorded outburst of the recurrent eclipsing nova USco was observed simultaneously in X-ra...
We present X-ray, UV, optical, and radio observations of the nearby ($\approx78$ Mpc) tidal disrupti...
Estimates of the accretion rate in symbiotic recurrent novae (RNe) often fall short of theoretical e...
We study the disk instability and the effect of irradiation on outbursts in the black hole X-ray nov...
RS Oph is a recurrent nova which began its latest outburst on 2006 Feb 12. Previous outbursts have s...
We present a comprehensive review of all observations of the eclipsing recurrent Nova LMC 1968 in th...
We report on the detection and analysis of extended X-ray emission by the Chandra X-ray Observatory ...
RS Ophiuchi is a recurrent nova system that experiences outbursts every ~20 years, implying accretio...
1ES 1927+654 is a paradigm-defying AGN and one of the most peculiar X-ray nuclear transients. In ear...
Nova LMC 2009a is confirmed as a Recurrent Nova (RN) from positional coincidence with nova LMC 1971b...
A sudden increase in the rate at which material reaches the most internal part of an accretion disk,...
The current superactive state of the recurrent nova T Coronae Borealis (T CrB) has been observed wit...
Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries in...
© 2022. The Author(s). Published by the American Astronomical Society. This is an open access articl...
Estimates of the accretion rate in symbiotic recurrent novae (RNe) often fall short of theoretical e...
The tenth recorded outburst of the recurrent eclipsing nova USco was observed simultaneously in X-ra...
We present X-ray, UV, optical, and radio observations of the nearby ($\approx78$ Mpc) tidal disrupti...
Estimates of the accretion rate in symbiotic recurrent novae (RNe) often fall short of theoretical e...
We study the disk instability and the effect of irradiation on outbursts in the black hole X-ray nov...
RS Oph is a recurrent nova which began its latest outburst on 2006 Feb 12. Previous outbursts have s...
We present a comprehensive review of all observations of the eclipsing recurrent Nova LMC 1968 in th...
We report on the detection and analysis of extended X-ray emission by the Chandra X-ray Observatory ...
RS Ophiuchi is a recurrent nova system that experiences outbursts every ~20 years, implying accretio...
1ES 1927+654 is a paradigm-defying AGN and one of the most peculiar X-ray nuclear transients. In ear...
Nova LMC 2009a is confirmed as a Recurrent Nova (RN) from positional coincidence with nova LMC 1971b...