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Corongiu, A. Possenti, A. Ridolfi, B. W. Stappers, E. D. Barr, F. Abbate, L. Vleeschower, L. Zhang, M. Bailes, M. Kramer, P. C. C. Freire, P. V. Padmanabh, S. Buchner, S. M. Ransom, V. Balakrishnan, V. Venkatraman Krishnan, W. Chen","submitted_at":"2024-03-18T18:00:14Z","abstract_excerpt":"Using MeerKAT, we have discovered three new millisecond pulsars (MSPs) in the bulge globular cluster M62: M62H, M62I, and M62J. All three are in binary systems, which means all ten known pulsars in the cluster are in binaries. M62H has a planetary-mass companion with a median mass $M_{\\rm c,med} \\sim 3$ M$_{\\rm J}$ and a mean density of $\\rho \\sim 11$ g cm$^{-3}$. M62I has an orbital period of 0.51 days and a $M_{\\rm c,med} \\sim 0.15$ M$_{\\odot}$. Neither of these low-mass systems exhibit eclipses. 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