The extremely rapid rotational braking of the magnetic helium-strong star HD 37776

Z Mikulášek, J Krtička, GW Henry, J Zverko… - Astronomy & …, 2008 - aanda.org
Context. Light and spectrum variations of the magnetic chemically peculiar (mCP) stars are
explained by the oblique rigid rotator model with a rotation period usually assumed to be …

A White Dwarf–Main-sequence Binary Unveiled by Time-domain Observations from LAMOST and TESS

LL Zheng, WM Gu, M Sun, ZX Zhang, T Yi… - The Astrophysical …, 2022 - iopscience.iop.org
We report a single-lined white dwarf–main-sequence binary system, LAMOST J172900. 17+
652952.8, which is discovered by the Large Sky Area Multi-Object Fibre Spectroscopic …

Orbital and atmospheric parameters of two wide O-type subdwarf binaries: BD− 11o162 and Feige 80

F Molina, J Vos, P Németh, R Østensen… - Astronomy & …, 2022 - aanda.org
Context. There are 23 long-period binary systems discovered to date that contain a B-type
hot subdwarf whose orbital parameters have been fully solved. They evolve into O-type …

Hot subdwarf wind models with accurate abundances-II. Helium-dominated merger products CD–46 8926 and CD–51 11879

J Krtička, I Krtičková, J Janík, P Németh, J Kubát… - Astronomy & …, 2024 - aanda.org
Context. Helium-dominated subdwarfs are core helium burning stars stripped of their
envelope. The nuclear evolution of these stars alters surface abundances. Modified …

The nature of medium-period variables on the extreme horizontal branch-I. X-shooter study of variable stars in the globular cluster ω Cen

J Krtička, I Krtičková, CM Bidin, M Kajan… - Astronomy & …, 2024 - aanda.org
A fraction of the extreme horizontal branch stars of globular clusters exhibit a periodic light
variability that has been attributed to rotational modulation caused by surface spots. These …

A multi-method approach to radial-velocity measurement for single-object spectra

M David, R Blomme, Y Frémat, Y Damerdji… - Astronomy & …, 2014 - aanda.org
Context. The derivation of radial velocities from large numbers of spectra that typically result
from survey work, requires automation. However, except for the classical cases of slowly …

Mining Double-line Spectroscopic Candidates in the LAMOST Medium-resolution Spectroscopic Survey Using a Human–AI Hybrid Method

S Li, C Li, C Li, D Fan, Y Xu, L Mi… - The Astrophysical …, 2024 - iopscience.iop.org
We utilize a hybrid approach that integrates the traditional cross-correlation function (CCF)
and machine learning to detect spectroscopic multiple star systems, specifically focusing on …

Hot subdwarf wind models with accurate abundances-I. Hydrogen dominated stars HD 49798 and BD+ 18° 2647

J Krtička, J Janík, I Krtičková, S Mereghetti… - Astronomy & …, 2019 - aanda.org
Context. Hot subdwarfs are helium burning objects in late stages of their evolution. These
subluminous stars can develop winds driven by light absorption in the lines of heavier …

EPIC 206197016: A very hot white dwarf orbited by a strongly irradiated red dwarf

J Krtička, A Kawka, Z Mikulášek, L Fossati… - Astronomy & …, 2023 - aanda.org
Context. Very precise satellite photometry has revealed a large number of variable stars
whose variability is caused either by surface spots or by binarity. Detailed studies of such …

Stars with discrepant v sin i as derived from the Ca II λ3933 Å and Mg II λ4481 Å lines. V. HD 182255 and HD 214923—SPB stars in binary systems

J Zverko, I Romanyuk, I Iliev, D Kudryavtsev… - Astrophysical …, 2016 - Springer
The axial rotation of a star plays an important role in its evolution, the physical conditions in
its atmosphere and the appearance of its spectrum. We analyzed the CCD spectra of two …