output
20062026
most citedThe James Webb Space Telescope Mission

490 citations

Showing astro-ph.SRShow all

18 papers · 1 filter

astro-ph.SR2022★ 5 cited

Detection of cesium in the atmosphere of the hot He-rich white dwarf HD 149499B

P. Chayer, C. Mendoza, M. Meléndez +2

We report the first detection of cesium (Z = 55) in the atmosphere of a white dwarf. Around a dozen absorption lines of Cs IV, Cs V, and Cs VI have been identified in the Far Ultra…

astro-ph.SR2013★ 98 cited

Seismic constraints on rotation of Sun-like star and mass of exoplanet

Laurent Gizon, Jérome Ballot, Eric Michel +32

Rotation is thought to drive cyclic magnetic activity in the Sun and Sun-like stars. Stellar dynamos, however, are poorly understood owing to the scarcity of observations of rotati…

astro-ph.SR2012★ 59 cited

Torsional Oscillations in a Global Solar Dynamo

P. Beaudoin, P. Charbonneau, E. Racine +1

We characterize and analyze rotational torsional oscillations developing in a large-eddy magnetohydrodynamical simulation of solar convection (Ghizaru, Charbonneau, and Smolarkiewi…

astro-ph.SR2012★ 31 cited

Precise Modeling of the Exoplanet Host Star and CoRoT Main Target HD 52265

M. E. Escobar, S. Théado S. Vauclair, J. Ballot +8

This paper presents a detailed and precise study of the characteristics of the Exoplanet Host Star and CoRoT main target HD 52265, as derived from asteroseismic studies. The result…

astro-ph.SR2012★ 19 cited

Hubble Space Telescope FUV Spectra of the Post-Common-Envelope Hyades Binary V471 Tauri

E. M. Sion, H. E. Bond, D. Lindler +4

We have carried out an analysis of the HST STIS archival spectra of the magnetic white dwarf in the Hyades eclipsing-spectroscopic, post-common envelope binary V471 Tauri, time res…

astro-ph.SR2012★ 222 cited

Accurate parameters of 93 solar-type Kepler targets

H. Bruntt, S. Basu, B. Smalley +29

We present a detailed spectroscopic study of 93 solar-type stars that are targets of the NASA/Kepler mission and provide detailed chemical composition of each target. We find that…