206 citations · 326 across the 5 of their papers we have counts for
5 papers
Star formation in a high-pressure environment: An SMA view of the Galactic centre dust ridge
D. L. Walker, S. N. Longmore, Q. Zhang +14
The star formation rate in the Central Molecular Zone (CMZ) is an order of magnitude lower than predicted according to star formation relations that have been calibrated in the dis…
Variability Of The Magnetic Field Power Spectrum In The Solar Wind At Electron Scales
Owen Roberts, Olga Alexandrova, Primoz Kajdic +4
At the electron scales the power spectrum of solar-wind magnetic fluctuations can be highly variable and the dissipation mechanisms of the magnetic energy into the various particle…
The link between solenoidal turbulence and slow star formation in G0.253+0.016
C. Federrath, J. M. Rathborne, S. N. Longmore +8
Star formation in the Galactic disc is primarily controlled by gravity, turbulence, and magnetic fields. It is not clear that this also applies to star formation near the Galactic…
The link between turbulence, magnetic fields, filaments, and star formation in the Central Molecular Zone cloud G0.253+0.016
C. Federrath, J. M. Rathborne, S. N. Longmore +8
Star formation is primarily controlled by the interplay between gravity, turbulence, and magnetic fields. However, the turbulence and magnetic fields in molecular clouds near the G…
Investigating Variability of Quiescent Neutron Stars in the Globular Clusters NGC 6440 and Terzan 5
A. R. Walsh, E. M. Cackett, F. Bernardini
The quiescent spectrum of neutron star low-mass X-ray binaries typically consists of two components - a thermal component associated with emission from the neutron star surface, an…