WISE J0909+0002 shows a 660-689 day rest-frame quasi-periodic optical oscillation, interpreted as Doppler-boosted emission from a supermassive black hole binary.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The possible long-term periodic variability of the extremely luminous quasar WISE J090924.01+000211.1
WISE J0909+0002 shows a 660-689 day rest-frame quasi-periodic optical oscillation, interpreted as Doppler-boosted emission from a supermassive black hole binary.