Search for multiwavelength emission from the binary millisecond pulsar PSR J1836-2354A in the globular cluster M22
arXiv:1904.07648 · doi:10.1093/mnras/stz1100
Abstract
We present a multi-band search for X-ray, optical and -ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular cluster M22. X-ray emission is significantly detected in two Chandra observations, performed in 2005 and 2014, at a luminosity of 2-310 erg s, in the 0.5-8 keV energy range. The radio and the X-ray source positions are found consistent within 1 error box. No detection is found in archival XMM-Newton and Swift/XRT observations, compatible with the Chandra flux level. The low statistics prevents us to assess if the X-ray source varied between the two observations. The X-ray spectrum is consistent with a power-law of photon index 1.5. We favour as the most probable origin of the X-ray emission an intrabinary shock scenario. We searched for optical and -ray counterparts to the radio source using data from Hubble Space Telescope and Fermi-LAT catalogues, respectively. No optical counterpart down to V=25.9 and I=24.7 (3) is detected, which suggests a companion mass of 0.1-0.2 . Combined with the low X-ray luminosity, this is consistent with a black widow nature of PSR J1636-2354A. Inspecting the 8-year Fermi-LAT catalogue, we found a -ray source, 4FGL J1836.8-2354, with a positional uncertainty consistent with the globular cluster, but not with the radio position of the millisecond pulsar.
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