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• W2050067092 abstract "We report the detection of a new 3.06 ms binary pulsar in the globular cluster NGC 6544 using a Fourier-domain acceleration search. With an implied companion mass of ~0.01 M☉ and an orbital period of only Pb ~ 1.7 hr, it displays orbital properties very similar to many pulsars that are eclipsed by their companion winds. The orbital period is the second shortest of known binary pulsars after 47 Tuc R. The measured flux density of 1.3 ± 0.4 mJy at 1332 MHz indicates that the pulsar is almost certainly the known steep-spectrum point source near the core of NGC 6544." @default.
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• W2050067092 date "2001-01-01" @default.
• W2050067092 modified "2023-09-22" @default.
• W2050067092 title "A Binary Millisecond Pulsar in Globular Cluster NGC 6544" @default.
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• W2050067092 doi "https://doi.org/10.1086/318062" @default.
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