A new ALMA-based dynamical model confirms the central black hole of NGC 7052 weighs about 2.5 billion solar masses and revises the galaxy's I-band stellar mass-to-light ratio down by 10%.
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Revisiting the supermassive black hole mass of NGC 7052 using high spatial resolution molecular gas observed with ALMA
A new ALMA-based dynamical model confirms the central black hole of NGC 7052 weighs about 2.5 billion solar masses and revises the galaxy's I-band stellar mass-to-light ratio down by 10%.