Analysis of eight magnetic chemically peculiar stars with rotational modulation
Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) has provided stellar
photometry to the astronomical community. We have used TESS data to study rotational …
photometry to the astronomical community. We have used TESS data to study rotational …
TESS Cycle 2 observations of roAp stars with 2-min cadence data
DL Holdsworth, MS Cunha… - Monthly Notices of …, 2024 - academic.oup.com
We present the results of a systematic search of the Transiting Exoplanet Survey Satellite
(TESS) 2-min cadence data for new rapidly oscillating Ap (roAp) stars observed during the …
(TESS) 2-min cadence data for new rapidly oscillating Ap (roAp) stars observed during the …
The nature of medium-period variables on the extreme horizontal branch-I. X-shooter study of variable stars in the globular cluster ω Cen
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 …
variability that has been attributed to rotational modulation caused by surface spots. These …
Understanding the rotational variability of K2 targets-HgMn star KIC 250152017 and blue horizontal branch star KIC 249660366
Context. Ultraprecise space photometry enables us to reveal light variability even in stars
that were previously deemed constant. A large group of such stars show variations that may …
that were previously deemed constant. A large group of such stars show variations that may …
Magnetic Fields of Chemically Peculiar and Related Stars. 5. Main Results of 2018 and Near-Future Prospects
II Romanyuk - Astrophysical Bulletin, 2019 - Springer
We have surveyed about a hundred papers published in 2018 in the leading astronomical
journals and related to the “Magnetic fields and physical parameters of chemically peculiar …
journals and related to the “Magnetic fields and physical parameters of chemically peculiar …
Revealing the nature of HD63401
HD~ 63401 is known magnetic chemically peculiar (mCP) star that shows a slow rotation
and probably possesses a hydrodynamically stable stellar atmosphere. In the latter case the …
and probably possesses a hydrodynamically stable stellar atmosphere. In the latter case the …
[PDF][PDF] Understanding the rotational variability of K2 targets
Context. Ultraprecise space photometry enables us to reveal light variability even in stars
that were previously deemed constant. A large group of such stars show variations that may …
that were previously deemed constant. A large group of such stars show variations that may …
VeSElkA: Vertical Stratification of Element Abundances in CP stars
A portion of the upper main-sequence stars, called chemically peculiar (CP) stars, show
significant abundance anomalies mainly due to atomic diffusion of chemical elements within …
significant abundance anomalies mainly due to atomic diffusion of chemical elements within …
Магнитные поля химически пекулярных и родственных им звезд. 5. Основные результаты 2018 года и анализ ближайших перспектив
ИИ Романюк - Астрофизический бюллетень, 2019 - cyberleninka.ru
Приводится обзор около сотни работ, выполненных по теме «Магнитные поля и
физические параметры химически пекулярных и родственных им звезд « …
физические параметры химически пекулярных и родственных им звезд « …