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Geoffrey C. Clayton

4 papers hereh-index 313 citations7 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • Geoffrey C. Clayton — 5 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.SR2025

Oxygen Isotope Ratios in Hydrogen-Deficient Carbon Stars: A Correlation with Effective Temperature and Implications for White Dwarf Merger Outcomes

Advait Mehla, Mansi M. Kasliwal, Viraj Karambelkar +5

Hydrogen-deficient Carbon (HdC) stars are a class of supergiants with anomalous chemical compositions, suggesting that they are remnants of CO-He white dwarf (WD) mergers. This cla…

astro-ph.SR2025

A Comprehensive Study of the Dust Declines in R Coronae Borealis Stars

Courtney L. Crawford, Jamie Soon, Geoffrey C. Clayton +4

The R Coronae Borealis (RCB) variables are rare, hydrogen-deficient, carbon-rich supergiants known for large, erratic declines in brightness due to dust formation. Recently, the nu…

astro-ph.SR2024

Hydrodynamic simulations of WD-WD mergers and the origin of RCB stars

Sagiv Shiber, Orsola De Marco, Patrick M. Motl +10

We study the properties of double white dwarf (DWD) mergers by performing hydrodynamic simulations using the new and improved adaptive mesh refinement code Octo-Tiger. We follow th…

astro-ph.SR2024

Modelling Hydrogen-deficient Carbon stars in MESA -- The effects of total mass and mass ratio

Courtney L. Crawford, Nikita Nikultsev, Geoffrey C. Clayton +3

Hydrogen-deficient Carbon (HdC) stars are rare, low-mass, chemically peculiar, supergiant variables believed to be formed by a double white dwarf (DWD) merger, specifically of a Ca…

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