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2019MNRAS.489.2069S - Mon. Not. R. Astron. Soc., 489, 2069-2078 (2019/October-3)

Lack of close-in, massive planets of main-sequence A-type stars from Kepler.

SABOTTA S., KABATH P., KORTH J., GUENTHER E.W., DUPKALA D., GRZIWA S., KLOCOVA T. and SKARKA M.

Abstract (from CDS):

Some theories of planet formation and evolution predict that intermediate-mass stars host more hot Jupiters than Sun-like stars, others reach the conclusion that such objects are very rare. By determining the frequencies of those planets we can test those theories.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: photometric - techniques: spectroscopic - stars: activity - stars: oscillations - planetary systems

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

CDS comments: p.2073: KOI-7733 not identified.

Simbad objects: 25

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2021.01.18-05:54:19

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