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20022009
most citedThe case for a distributed solar dynamo shaped by near-surface shear

406 citations

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31 papers · 1 filter

astro-ph20072 cited

Why coronal mass ejections are necessary for the dynamo

Axel Brandenburg

Large scale dynamo-generated fields are a combination of interlocked poloidal and toroidal fields. Such fields possess magnetic helicity that needs to be regenerated and destroyed…

astro-ph200747 cited

Impact of nuclear "pasta" on neutrino transport in collapsing stellar cores

Hidetaka Sonoda, Gentaro Watanabe, Katsuhiko Sato +3

Nuclear ``pasta'', nonspherical nuclei in dense matter, is predicted to occur in collapsing supernova cores. We show how pasta phases affect the neutrino transport cross section vi…

astro-ph200614 cited

RApid Temporal Survey - RATS II: Followup observations of 4 newly discovered short period variables

Gavin Ramsay, Ralf Napiwotzki, Pasi Hakala +1

The RApid Temporal Survey (RATS) is a survey to detect objects whose optical intensity varies on timescales of less than ~70 min. In our pilot dataset taken with the INT and the Wi…

astro-ph200624 cited

Can the thermal instability drive turbulence?

Axel Brandenburg, Maarit J. Korpi, Antony J. Mee

The thermal instability with a piecewise power law cooling function is investigated using one- and three-dimensional simulations with periodic and shearing-periodic boundary condit…

astro-ph200648 cited

Primordial Stellar Feedback and the Origin of Hyper Metal-Poor Stars

Torgny Karlsson

The apparent absence of stars in the Milky Way halo with -5 ~< [Fe/H] ~< -4 suggests that the gas out of which the halo stars were born experienced a period of low or delayed star…

astro-ph200659 cited

Turbulence from localized random expansion waves

Antony J. Mee, Axel Brandenburg

In an attempt to determine the outer scale of turbulence driven by localized sources, such as supernova explosions in the interstellar medium, we consider a forcing function given…