activity
20102023
most citedThe stellar rotation--activity relationship in fully convective M dwarfs

284 citations · 1.6k across the 29 of their papers we have counts for

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15 papers · 1 filter

astro-ph.SR2022

Coronal and chromospheric emission in A-type stars

Hans Moritz Günther, Carl Melis, J. Robrade +3

Cool stars on the main sequence generate X-rays from coronal activity, powered by a convective dynamo. With increasing temperature, the convective envelope becomes smaller and X-ra…

astro-ph.SR2020★ 22 cited

An Earth-like stellar wind environment for Proxima Centauri c

Julián D. Alvarado-Gómez, Jeremy J. Drake, Cecilia Garraffo +4

A new planet has been recently discovered around Proxima Centauri. With an orbital separation of au and a minimum mass of about , Proxima c is a prime…

astro-ph.SR2020★ 42 cited

Tuning the Exo-Space Weather Radio for Stellar Coronal Mass Ejections

Julián D. Alvarado-Gómez, Jeremy J. Drake, Federico Fraschetti +7

Coronal mass ejections (CMEs) on stars other than the Sun have proven very difficult to detect. One promising pathway lies in the detection of type II radio bursts. Their appearanc…

astro-ph.SR2019

(Simulating) Coronal Mass Ejections in Active Stars

Julián D. Alvarado-Gómez, Jeremy J. Drake, Cecilia Garraffo +4

The stellar magnetic field completely dominates the environment around late-type stars. It is responsible for driving the coronal high-energy radiation (e.g. EUV/X-rays), the devel…

astro-ph.SR2019★ 57 cited

Coronal response to magnetically-suppressed CME events in M-dwarf stars

Julián D. Alvarado-Gómez, Jeremy J. Drake, Sofia P. Moschou +4

We report the results of the first state-of-the-art numerical simulations of Coronal Mass Ejections (CMEs) taking place in realistic magnetic field configurations of moderately act…

astro-ph.SR2019

Magnetism in the Brown Dwarf Regime

Melodie M. Kao, J. Sebastian Pineda, Peter Williams +8

A suite of discoveries in the last two decades demonstrate that we are now at a point where incorporating magnetic behavior is key for advancing our ability to characterize substel…

astro-ph.SR2019★ 1 cited

Astro2020 Science White Paper: Fundamental Physics with Brown Dwarfs: The Mass-Radius Relation

Adam Burgasser, Isabelle Baraffe, Matthew Browning +17

The lowest-mass stars, brown dwarfs and giant exoplanets span a minimum in the mass-radius relationship that probes the fundamental physics of extreme states of matter, magnetism,…

astro-ph.SR2018★ 284 cited

The stellar rotation--activity relationship in fully convective M dwarfs

Nicholas J. Wright, Elisabeth R. Newton, Peter K. G. Williams +2

The coronal activity-rotation relationship is considered to be a proxy for the underlying stellar dynamo responsible for magnetic activity in solar and late-type stars. While this…

astro-ph.SR2016★ 63 cited

Magnetic cycles in a dynamo simulation of fully convective M-star Proxima Centauri

Rakesh K. Yadav, Ulrich R. Christensen, Scott J. Wolk +1

The recent discovery of an Earth-like exoplanet around Proxima Centauri has shined a spot light on slowly rotating fully convective M-stars. When such stars rotate rapidly (period…

astro-ph.SR2016★ 13 cited

Giant coronal loops dominate the quiescent X-ray emission in rapidly rotating M stars

O. Cohen, R. Yadav, C. Garraffo +5

Observations indicate that magnetic fields in rapidly rotating stars are very strong, on both small and large scales. What is the nature of the resulting corona? Here we seek to sh…

astro-ph.SR2015★ 134 cited

Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

Rakesh K. Yadav, Ulrich R. Christensen, Julien Morin +4

Despite the lack of a shear-rich tachocline region low-mass fully convective stars are capable of generating strong magnetic fields, indicating that a dynamo mechanism fundamentall…

astro-ph.SR2014★ 61 cited

Formation of starspots in self-consistent global dynamo models: Polar spots on cool stars

Rakesh K. Yadav, Thomas Gastine, Ulrich R. Christensen +1

Observations of cool stars reveal dark spot-like features on their surfaces. Compared to sunspots, starspots can be bigger or cover a larger fraction of the stellar surface. While…

astro-ph.SR2013★ 205 cited

From solar-like to anti-solar differential rotation in cool stars

T. Gastine, R. K. Yadav, J. Morin +2

Stellar differential rotation can be separated into two main regimes: solar-like when the equator rotates faster than the poles and anti-solar when the polar regions rotate faster…

astro-ph.SR2013

Bridging planets and stars using scaling laws in anelastic spherical shell dynamos

Rakesh K. Yadav, Thomas Gastine, Ulrich R. Christensen +1

Dynamos operating in the interiors of rapidly rotating planets and low-mass stars might belong to a similar category where rotation plays a vital role. We quantify this similarity…

astro-ph.SR2013★ 55 cited

Consistent scaling laws in anelastic spherical shell dynamos

Rakesh K. Yadav, Thomas Gastine, Ulrich R. Christensen +1

Numerical dynamo models always employ parameter values that differ by orders of magnitude from the values expected in natural objects. However, such models have been successful in…