Abstract We present new spectroscopic data for Gaia DR3 2309499817384726016 (WD 0008-350A) and its two wide, comoving, low-mass companions. We confirm the white dwarf is a hydrogen rich DA, with T eff = 6200 ± 90 K and a mass of 0.63 ± 0.03 M ⊙ , close to that of the average white dwarf. Near-infrared spectra of the two stellar companions to WD 0008-350A reveal that the inner companion is an M dwarf, exhibiting a spectral type of M8. Furthermore, the outer companion is identified as a possible M6 + M9 binary. This paper examines the evidence which suggests the system may be quadruple.
Building similarity graph...
Analyzing shared references across papers
Loading...
Peter A. Jałowiczor
University of Sheffield
Thomas P. Bickle
J. Davy Kirkpatrick
SHILAP Revista de lepidopterología
The Astronomical Journal
Building similarity graph...
Analyzing shared references across papers
Loading...
Jałowiczor et al. (Wed,) studied this question.
synapsesocial.com/papers/69994ba9873532290d01fd70 — DOI: https://doi.org/10.3847/1538-3881/ae38d3