most citedCarbon star formation as seen through the non-monotonic initial-final mass relation

91 citations · 125 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2020

An Increase in Small-planet Occurrence with Metallicity for Late-type Dwarf Stars in the Kepler Field and Its Implications for Planet Formation

Cicero X. Lu, Kevin C. Schlaufman, Sihao Cheng

While it is well established that giant-planet occurrence rises rapidly with host star metallicity, it is not yet clear if small-planet occurrence around late-type dwarf stars depe…

astro-ph.SR2020

Multi-Gigayear White Dwarf Cooling Delays from Clustering-Enhanced Gravitational Sedimentation

Evan B. Bauer, Josiah Schwab, Lars Bildsten +1

Cooling white dwarfs (WDs) can yield accurate ages when theoretical cooling models fully account for the physics of the dense plasma of WD interiors. We use MESA to investigate coo…

astro-ph.SR202034 cited

A Gravitational Redshift Measurement of the White Dwarf Mass-Radius Relation

Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska +1

The mass-radius relation of white dwarfs is largely determined by the equation of state of degenerate electrons, which causes the stellar radius to decrease as mass increases. Here…

astro-ph.SR202091 cited

Carbon star formation as seen through the non-monotonic initial-final mass relation

Paola Marigo, Jeffrey D. Cummings, Jason Lee Curtis +13

The initial-final mass relation (IFMR) links the birth mass of a star to the mass of the compact remnant left at its death. While the relevance of the IFMR across astrophysics is u…

astro-ph.SR2020

Two delays in white dwarf evolution revealed by Gaia

Sihao Cheng

By comparing two age indicators of high-mass white dwarfs derived from Gaia data, two discoveries have been made recently: one is the existence of a cooling anomaly that produces t…