X-ray and Radio Studies of the candidate Millisecond Pulsar Binary 4FGL J0935.3+0901
arXiv:2111.15089 · doi:10.1088/1674-4527/ac3e5e
Abstract
4FGL J0935.5+0901, a -ray source recently identified as a candidate redback-type millisecond pulsar binary (MSP), shows an interesting feature of having double-peaked emission lines in its optical spectrum. The feature would further suggest the source as a transitional MSP system in the sub-luminous disk state. We have observed the source with \xmm\ and Five-hundred-meter Aperture Spherical radio Telescope (FAST) at X-ray and radio frequencies respectivelyfor further studies. From the X-ray observation, a bimodal count-rate distribution, which is a distinctive feature of the transitional MSP systems, is not detected, while the properties of X-ray variability and power-law spectrum are determined for the source. These results help establish the consistency of it being a redback in the radio pulsar state. However no radio pulsation signals are found in the FAST observation, resulting an upper limit on the flux density of Jy. Implications of these results are discussed.
10 pages, 5 figures
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