Results 51 to 60 of about 215 (139)
Near-infrared CO molecular lines are suggested to be linked with dynamic processes in post–asymptotic giant branch (post-AGB) stars; however, they have not been investigated at high spectral resolution.
Kārlis Puķītis
doaj +1 more source
Variable Stars in M31 Stellar Clusters from the Panchromatic Hubble Andromeda Treasury
Variable stars in stellar clusters can offer key constraints on stellar evolution and pulsation models, utilizing estimates of host cluster properties to constrain stellar physical parameters.
Richard Smith +11 more
doaj +1 more source
The interactions between post–asymptotic giant branch (post-AGB) binaries and their circumbinary disks play a central role in shaping the evolution of these systems.
Maksym Mohorian +12 more
doaj +1 more source
Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts
The recently identified Gaia population of main-sequence–white dwarf (MS+WD) binaries at separations of ∼1 au, often with moderate eccentricities, is not readily reproduced by binary population synthesis models.
Param Rekhi +6 more
doaj +1 more source
We report the discovery of LAMOST J0041+3948, the most luminous post-asymptotic giant-branch (AGB) Type II Cepheid known, located in the Andromeda Giant Stellar Stream.
Pinjian Chen +9 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
A Deficit of Massive White Dwarfs in Gaia Astrometric Binaries
The third data release of Gaia introduced a large catalog of astrometric binaries, out of which about 3200 are likely main-sequence stars with a white dwarf (WD) companion.
Na’ama Hallakoun +4 more
doaj +1 more source
Observations of the Halo Star HD 177566
We have analyzed archival far-ultraviolet (FUV) and optical spectra of the hot halo star HD 177566. The star has an effective temperature T _eff = 33,000 ± 1000 K, surface gravity $\mathrm{log}g=3.79\pm 0.11$ , and helium abundance $\mathrm{log}N({\rm{He}
William V. Dixon, Pierre Chayer
doaj +1 more source
CO observations in rotating circumbinary post-AGB disks
Context. There is a group of post-asymptotic giant branch (post-AGB) stars that are part of a binary system and that show a significant infrared excess.
Gallardo Cava I. +5 more
doaj +1 more source

