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91̽»¨
Black Hole

Lensing of space time around a black hole. At 91̽»¨ we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Arun Kumar Naidu

Visitor

Sub department

  • Astrophysics
arun.naidu@physics.ox.ac.uk
Telephone: 01865 273364
Denys Wilkinson Building, room 603D
  • About
  • Publications

First Discovery of New Pulsars and RRATs with CHIME/FRB

The Astrophysical Journal American Astronomical Society 922:1 (2021) 43

Authors:

DC Good, BC Andersen, P Chawla, K Crowter, FQ Dong, E Fonseca, BW Meyers, C Ng, Z Pleunis, SM Ransom, IH Stairs, CM Tan, M Bhardwaj, PJ Boyle, M Dobbs, BM Gaensler, VM Kaspi, KW Masui, A Naidu, M Rafiei-Ravandi, P Scholz, KM Smith, SP Tendulkar

Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620

The Astrophysical Journal Letters American Astronomical Society 915:1 (2021) l12

Authors:

E Fonseca, HT Cromartie, TT Pennucci, PS Ray, A Yu Kirichenko, SM Ransom, PB Demorest, IH Stairs, Z Arzoumanian, L Guillemot, A Parthasarathy, M Kerr, I Cognard, PT Baker, H Blumer, PR Brook, M DeCesar, T Dolch, FA Dong, EC Ferrara, W Fiore, N Garver-Daniels, DC Good, R Jennings, ML Jones, VM Kaspi, MT Lam, DR Lorimer, J Luo, A McEwen, JW McKee, MA McLaughlin, N McMann, BW Meyers, A Naidu, C Ng, DJ Nice, N Pol, HA Radovan, B Shapiro-Albert, CM Tan, SP Tendulkar, JK Swiggum, HM Wahl, WW Zhu

The CHIME Pulsar Project: System Overview

The Astrophysical Journal Supplement Series American Astronomical Society 255:1 (2021) 5

Authors:

M Amiri, KM Bandura, PJ Boyle, C Brar, J-F Cliche, K Crowter, D Cubranic, PB Demorest, NT Denman, M Dobbs, FQ Dong, M Fandino, E Fonseca, DC Good, M Halpern, AS Hill, C Höfer, VM Kaspi, TL Landecker, C Leung, H-H Lin, J Luo, KW Masui, JW McKee, J Mena-Parra, BW Meyers, D Michilli, A Naidu, L Newburgh, C Ng, C Patel, T Pinsonneault-Marotte, SM Ransom, A Renard, P Scholz, JR Shaw, AE Sikora, IH Stairs, CM Tan, SP Tendulkar, I Tretyakov, K Vanderlinde, H Wang, X Wang

High precision measurements of interstellar dispersion measure with the upgraded GMRT⋆

Astronomy & Astrophysics EDP Sciences 651 (2021) a5

Authors:

MA Krishnakumar, PK Manoharan, BC Joshi, R Girgaonkar, S Desai, M Bagchi, K Nobleson, L Dey, A Susobhanan, SC Susarla, MP Surnis, Y Maan, A Gopakumar, A Basu, ND Batra, A Choudhary, K De, Y Gupta, AK Naidu, D Pathak, J Singha, T Prabu

LOFAR Detection of 110–188 MHz Emission and Frequency-dependent Activity from FRB 20180916B

The Astrophysical Journal Letters American Astronomical Society 911:1 (2021) L3-L3

Authors:

Z Pleunis, D Michilli, CG Bassa, JWT Hessels, A Naidu, BC Andersen, P Chawla, E Fonseca, A Gopinath, VM Kaspi, VI Kondratiev, DZ Li, M Bhardwaj, PJ Boyle, C Brar, T Cassanelli, Y Gupta, A Josephy, R Karuppusamy, A Keimpema, F Kirsten, C Leung, B Marcote, KW Masui, R Mckinven

Abstract:

Fast radio bursts (FRBs) are transient radio signals with millisecond-duration, large dispersion measure (DM) and extremely high brightness temperature. Among them, FRB 20180916B has been found to have a 16-day periodic activity. However, the physical origin of the periodicity is still a mystery. Here, we utilize the comprehensive observational data to diagnose the periodic models. We find that the ultra-long rotation model is the most probable one for the periodic activity. However, this model cannot reproduce the observed rotation measure (RM) variations. We propose a self-consistent model, i.e., a massive binary containing a slowly rotational neutron star and a massive star with large mass loss, which can naturally accommodate the wealth of observational features for FRB 20180916B. In this model, the RM variation is periodic, which can be tested by future observations.Comment: 12 pages, 8 figure

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