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19922026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2018 · astro-ph.SRShow all

29 papers · 2 filters

astro-ph.SR2018★ 20 cited

Expansion of High Speed Solar Wind Streams from Coronal Holes through the Inner Heliosphere

Tadhg M. Garton, Sophie A. Murray, Peter T. Gallagher

Coronal holes (CHs) are regions of open magnetic flux which are the source of high speed solar wind (HSSW) streams. To date, it is not clear which aspects of CHs are of most influe…

astro-ph.SR2018★ 51 cited

Direct evidence of a full dipole flip during the magnetic cycle of a sun-like star

S. Boro Saikia, T. Lueftinger, S. V Jeffers +9

The behaviour of the large-scale dipolar field, during a star's magnetic cycle, can provide valuable insight into the stellar dynamo and associated magnetic field manifestations su…

astro-ph.SR2018★ 32 cited

The diversity of supernovae and impostors shortly after explosion

I. Boian, J. H. Groh

Observational surveys are now able to detect an increasing number of transients, such as core-collapse supernovae (SN) and powerful non-terminal outbursts (SN impostors). Dedicated…

astro-ph.SR2018★ 48 cited

Observing the simulations: Applying ZDI to 3D non-potential magnetic field simulations

L. T. Lehmann, G. A. J. Hussain, M. M. Jardine +2

The large-scale magnetic fields of stars can be obtained with the Zeeman-Doppler-Imaging (ZDI) technique, but their interpretation is still challenging as the contribution of the s…

astro-ph.SR2018★ 18 cited

The Rotationally Modulated Polarization of Boo A

Daniel V. Cotton, Dag Evensberget, Stephen C. Marsden +9

We have observed the active star Boo A (HD 131156A) with high precision broadband linear polarimetry contemporaneously with circular spectropolarimetry. We find both signals ar…

astro-ph.SR2018★ 30 cited

The Solar Wind in Time II: 3D stellar wind structure and radio emission

D. Ó Fionnagáin, A. A. Vidotto, P. Petit +5

In this work, we simulate the evolution of the solar wind along its main sequence lifetime and compute its thermal radio emission. To study the evolution of the solar wind, we use…