activity
20172022
most citedThe Stellar CME-flare relation: What do historic observations reveal?

132 citations · 440 across the 16 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.SR2018

Meter- to Millimeter Emission from Cool Stellar Systems: Latest Results, Synergies Across the Spectrum, and Outlook for the Next Decade

Jan Forbrich, Peter K. G. Williams, Emily Drabek-Maunder +12

Radio observations of cool stellar systems provide unique information on their magnetic fields, high-energy processes, and chemistry. Buoyed by powerful new instruments (e.g. ALMA,…

astro-ph.SR2018

The Magnetic Nature of the Cataclysmic Variable Period Gap

C. Garraffo, J. J. Drake, J. D. Alvarado-Gomez +2

One of the most important problems in the context of cataclysmic variables (CVs) is the lack of observations of systems with periods between 2 and 3.12 hours, known as the period g…

astro-ph.SR2018

Synthetic Radio Imaging for Quiescent and CME-flare Scenarios

Sofia-Paraskevi Moschou, Igor Sokolov, Ofer Cohen +5

Radio observations grant access to a wide range of physical processes through different emission mechanisms. These processes range from thermal and quiescent to eruptive phenomena,…

astro-ph.SR2018

Exoplanet Modulation of Stellar Coronal Radio Emission

Ofer Cohen, Sofia-Paraskevi Moschou, Alex Glocer +5

The search for exoplanets in the radio bands has been focused on detecting radio emissions produced by the interaction between magnetized planets and the stellar wind (auroral emis…

astro-ph.SR2018

Suppression of Coronal Mass Ejections in active stars by an overlying large-scale magnetic field: A numerical study

Julián D. Alvarado-Gómez, Jeremy J. Drake, Ofer Cohen +2

We present results from a set of numerical simulations aimed at exploring the mechanism of coronal mass ejection (CME) suppression in active stars by an overlying large-scale magne…

astro-ph.SR2018

The Revolution Revolution: magnetic morphology driven spin-down

C. Garraffo, J. J. Drake, A. Dotter +6

Observations of young open clusters show a bimodal distribution of rotation periods that has been difficult to explain with existing stellar spin-down models. Detailed MHD stellar…