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Nanda Rea

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Articles

A binary model of long-period radio transients and white dwarf pulsars - Nature Astronomy

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By Csanád Horváth, Nanda Rea, Natasha Hurley-Walker, Samuel J. McSweeney
| Nature Verified
Abstract Long-period radio transients (LPTs) represent a recently uncovered class of Galactic radio sources exhibiting minutes to hours periodicities and highly polarized pulses of seconds to minutes duration. Their phenomenology does not fit exactly in any other class, although it might resemble that of radio magnetars or white dwarf (WD) pulsars. Two LPTs with confirmed multi-wavelength counterparts have now been identified as WD – M dwarf binaries.
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A persistent bow shock in a diskless magnetized accreting white dwarf - Nature Astronomy

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By Simone Scaringi, Domitilla de Martino, Nanda Rea, David Buckley, Paul J. Groot, Anna McLeod, anna mcleod, Luke Parker Verified, Krystian Iłkiewicz, Sara E. Motta, Noel Castro Segura
| Nature Verified
Abstract Stellar bow shocks form when an outflow interacts with the interstellar medium. In white dwarfs accreting from a binary companion, outflows are associated with strong winds from the donor star, the accretion disk or a thermonuclear runaway explosion on the white dwarf surface. To date, only six accreting white dwarfs are known to harbour disk-wind-driven bow shocks that are not associated with thermonuclear explosions.
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Detection of X-ray emission from a bright long-period radio transient - Nature

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By Ziteng Wang, Nanda Rea, DAVID KAPLAN, Emil Lenc, Zorawar Wadiasingh, Andrew Zic, Apurba Kumar Bera, Paz Beniamini, A. J. Cooper, Tracy Clarke, J. R. Dawson, Marcin Glowacki, Natasha Hurley-Walker, S. J. McSweeney, Emil J. Polisensky, Wendy Peters, George Abi Younes, Keith Bannister, Manisha Caleb, Clancy W. James, Mansi Kasliwal, Kaya Mori, Stella Ocker, Miguel Pérez-Torres, Hao Qiu, Kovi Rose, Ryan Shannon, Fayin Wang, Yuanming Wang, Zhenyin Zhao, Laura N. Driessen, Tara Murphy, Joscha N. Jahns-Schindler
| Nature Verified
Abstract Recently, a class of long-period radio transients (LPTs) has been discovered, exhibiting emission thousands of times longer than radio pulsars1,2,3,4,5. These findings, enabled by advances in wide-field radio surveys, challenge existing models of rotationally powered pulsars. Proposed models include highly magnetized neutron stars6, white-dwarf pulsars7 and white-dwarf binary systems with low-mass companions8.
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