output
20152023
most citedA radio pulsing white dwarf binary star

215 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions

8 papers

astro-ph.SR2023

Magnetic Field Line Separation by Random Ballistic Decorrelation in Transverse Magnetic Turbulence

Chutima Yannawa, Peera Pongkitiwanichakul, David Ruffolo +2

The statistics of the magnetic field line separation provide insight into how a bundle of field lines spreads out and the dispersion of non-thermal particles in a turbulent environ…

astro-ph.SR2020★ 34 cited

Magnetic Field Line Random Walk and Solar Energetic Particle Path Lengths: Stochastic Theory and PSP/ISoIS Observation

R. Chhiber, W. H. Matthaeus, C. M. S. Cohen +21

Context:In 2020 May-June, six solar energetic ion events were observed by the Parker Solar Probe/ISoIS instrument suite at 0.35 AU from the Sun. From standard velocity-dispersion a…

physics.space-ph2020★ 16 cited

Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles

Rohit Chhiber, David Ruffolo, William H. Matthaeus +4

The random walk of magnetic field lines is an important ingredient in understanding how the connectivity of the magnetic field affects the spatial transport and diffusion of charge…

astro-ph.SR2018

Photometric Investigation of Novae T Pyx, BT Mon and V574 Pup at Quiescence by using the 2.4 m Thai National Telescope

Ritthichai Thipboon, Metichai Kaewrakmuk, Farung Surina +1

Recurrent novae (RNe) are novae with multiple recorded outbursts powered by a thermonuclear runaway. The outburst occurs on the surface of the white dwarf which accompanies with a…

astro-ph.SR2018

Evolution of V339 Del (Nova Del 2013) since 0.37 to 75 Days after Discovery

Y. Mueangkon, S. Khamrat, D. Suekong +5

We study the evolution of V339 Del (Nova Del 2013) during 0.37 to 75 days after discovery. Spectra from the Liverpool Telescope were collected and analysed to find velocity of ejec…

astro-ph.SR2016★ 215 cited

A radio pulsing white dwarf binary star

T. R. Marsh, B. T. Gänsicke, S. Hümmerich +23

White dwarfs are compact stars, similar in size to Earth but ~200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengt…

astro-ph.EP2016★ 110 cited

High-speed photometry of the disintegrating planetesimals at WD1145+017: evidence for rapid dynamical evolution

B. T. Gaensicke, A. Aungwerojwit, T. R. Marsh +11

We obtained high-speed photometry of the disintegrating planetesimals orbiting the white dwarf WD1145+017, spanning a period of four weeks. The light curves show a dramatic evoluti…

astro-ph.SR2015★ 20 cited

Nova light curves from the Solar Mass Ejection Imager (SMEI) - II. The extended catalog

R. Hounsell, M. J. Darnley, M. F. Bode +10

We present the results from observing nine Galactic novae in eruption with the Solar Mass Ejection Imager (SMEI) between 2004 and 2009. While many of these novae reached peak magni…