Constraints on Remnant Planetary Systems as a Function of Main-sequence Mass with HST/COS

Constraints on Remnant Planetary Systems as a Function of Main-sequence Mass with HST/COS

As the descendants of stars with masses less than 8 M _⊙ on the main sequence, white dwarfs provide a unique way to constrain planetary occurrence around intermediate-mass stars (spectral types BAF) that are otherwise difficult to measure with radial-velocity or transit surveys. We update the analys...

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Bibliographic Details
Main Authors: Lou Baya Ould Rouis, J. J. Hermes, Boris T. Gänsicke, Snehalata Sahu, Detlev Koester, P.-E. Tremblay, Dimitri Veras, Jay Farihi, Tyler M. Heintz, Nicola Pietro Gentile Fusillo, Seth Redfield
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
White dwarf stars
Exoplanets
Ultraviolet astronomy
Stellar kinematics
Online Access:https://doi.org/10.3847/1538-4357/ad86bb

Internet

https://doi.org/10.3847/1538-4357/ad86bb

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