no code implementations • 8 Dec 2020 • Evan Petrosky, Hsiang-Chih Hwang, Nadia L. Zakamska, Vedant Chandra, Matthew J. Hill
The time-series component of WISE is a valuable resource for the study of variable objects.
Time Series Analysis Solar and Stellar Astrophysics
no code implementations • 28 Jul 2020 • Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska, Sihao Cheng
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.
Solar and Stellar Astrophysics Astrophysics of Galaxies
1 code implementation • 22 Jul 2020 • Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska, Tamás Budavári
The spectroscopic features of white dwarfs are formed in the thin upper layer of their stellar photosphere.
Solar and Stellar Astrophysics