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Resource Record Summary

Catalog Service:
CaIIHK emission in stars with close-in planets

Short name: J/A+A/540/A82
IVOA Identifier: ivo://CDS.VizieR/J/A+A/540/A82
DOI (Digital Object Identifier): 10.26093/cds/vizier.35400082
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/540/A82
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2012 Aug 22 12:11:21Z
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Description


The planet-star interaction is manifested in many ways. It has been found that a close-in exoplanet causes small but measurable variability in the cores of a few lines in the spectra of several stars, which corresponds to the orbital period of the exoplanet. Stars with and without exoplanets may have different properties. The main goal of our study is to search for the influence that exoplanets might have on atmospheres of their host stars. Unlike the previous studies, we do not study changes in the spectrum of a host star or differences between stars with and without exoplanets. We aim to study a large number of stars with exoplanets and the current level of their chromospheric activity and to look for a possible correlation with the exoplanetary properties.

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under Cooperative Agreement AST0122449 with the Johns Hopkins University
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