output
20022026
most citedThe Gaia mission

7.1k citations

Showing 2015 · astro-ph.SRShow all

18 papers · 2 filters

astro-ph.SR2015

Stellar magnetic activity and their influence on the habitability of exoplanets

T. Lüftinger, M. Güdel, C. P. Johnstone

Stellar magnetism, explorable via polarimetry, is a crucial driver of activity, ionization, photodissociation, chemistry and winds in stellar environments. Thus it has an important…

astro-ph.SR2015★ 37 cited

Short-period stellar activity cycles with Kepler photometry

Oleksiy V. Arkhypov, Maxim L. Khodachenko, Helmut Lammer +3

We study the short-periodic component of stellar activity with a cycle periods Pcyc up to 1000 days using the Kepler mission photometry of fast-rotating (rotational periods from 1…

astro-ph.SR2015★ 48 cited

Helium signature in red giant oscillation patterns observed by Kepler

M. Vrard, B. Mosser, C. Barban +6

The space-borne missions CoRoT and Kepler have provided a large amount of precise photometric data. Among the stars observed, red giants show a rich oscillation pattern that allows…

astro-ph.SR2015★ 5 cited

Two-dimensional segmentation of small convective patterns in radiation hydrodynamics simulations

B. Lemmerer, D. Utz, A. Hanslmeier +4

Recent results from high-resolution solar granulation observations indicate the existence of a population of small granular cells that are smaller than 600 km in diameter. These sm…

astro-ph.SR2015★ 34 cited

Oxygen isotopic ratios in intermediate-mass red giants

Thomas Lebzelter, Oscar Straniero, Kenneth Hinkle +2

Context. The abundances of the three main isotopes of oxygen are altered in the course of the CNO-cycle. When the first dredge-up mixes the burning products to the surface, the nuc…

astro-ph.SR2015★ 251 cited

The Extreme Ultraviolet and X-Ray Sun in Time: High-Energy Evolutionary Tracks of a Solar-Like Star

Lin Tu, Colin P. Johnstone, Manuel Güdel +1

Aims. We aim to describe the pre-main sequence and main-sequence evolution of X-ray and extreme-ultaviolet radiation of a solar mass star based on its rotational evolution starting…