We present a timing solution for the 5.31 ms spider millisecond pulsar (MSP) J1242−4712, discovered with the GMRT. PSR J1242−4712 orbits a companion of minimum mass 0.08 M _⊙ with an orbital period of 7.7 hr and occupies a relatively unexplored region in
Ankita Ghosh +9 more
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FAST: Its Scientific Achievements and Prospects. [PDF]
Qian L +5 more
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Identifying Pulsar Candidates in Interferometric Radio Images Using Scintillation
Pulsars have been primarily detected by their narrow pulses or periodicity in time domain data. Interferometric surveys for pulsars are challenging due to the trade-off between beam sensitivity and beam size and the corresponding tradeoff between survey ...
Jitendra Salal +2 more
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Electromagnetic counterparts to massive black-hole mergers. [PDF]
Bogdanović T, Miller MC, Blecha L.
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A Binary Origin for Ultralong-period Radio Pulsars
We propose a possible binary evolution model for the formation of ultralong-period pulsars. The model involves two key stages: first, a neutron star (NS) in wide binaries undergoes an effective spin-down phase through wind-fed accretion from its massive ...
Ying-Han Mao +4 more
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PIC methods in astrophysics: simulations of relativistic jets and kinetic physics in astrophysical systems. [PDF]
Nishikawa K +3 more
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First post-Newtonian <i>N</i>-body problem in Einstein-Cartan theory with the Weyssenhoff fluid: equations of motion. [PDF]
Battista E, Falco V.
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Finding the Ionospheric Fluctuations Reflection in the Pulsar Signals' Characteristics Observed with LOFAR. [PDF]
Błaszkiewicz LP +6 more
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Reading signatures of supermassive binary black holes in pulsar timing array observations. [PDF]
Goncharov B +12 more
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Estimation of mass and radii for charged compact objects using a modified Chaplygin equation of state in the Buchdahl-I metric. [PDF]
Zahra A +4 more
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