Spatially resolved spectroscopy across stellar surfaces: I. using exoplanet transits to analyze 3-D stellar atmospheres
CONTEXT: High-precision stellar analyses require hydrodynamic modeling to interpret chemical abundances or oscillation modes. Exoplanet atmosphere studies require stellar background spectra to be known along the transit path while detection of Earth analogs require stellar microvariability to be und...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
2017
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| In: |
Arxiv
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| Online-Zugang: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1708.01616
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| Verfasserangaben: | Dainis Dravins, Hans-Günter Ludwig, Erik Dahlén, and Hiva Pazira |
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