activity
20112019
most citedRotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2

59 citations · 70 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR201959 cited

Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2

M. S. Cunha, V. Antoci, D. L. Holdsworth +36

We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the rotational and pulsational variability of magnetic chemically peculiar A-type stars. We an…

astro-ph.SR20176 cited

Pulsations and Period Variations of the Scuti Star AN Lyncis in a possible three-body system

Gang Li, Jianning Fu, Jie Su +5

Observations for the Scuti star AN Lyn have been made between 2008 and 2016 with the 85-cm telescope at Xinglong station of National Astronomical Observatories of China, the 84…

astro-ph.SR20174 cited

Asteroseismology of the ultramassive ZZ Ceti star WD 0246+326

Chun Li, Jianning Fu, Lester Fox-Machado +2

The internal structures of pulsating white dwarfs can be explored only with asteroseismology. Time series photometric observations were made for the pulsating DA white dwarf (ZZ Ce…

astro-ph.SR2016

ROTSE1 J164341.65+251748.1: a new W UMa-type eclipsing binary

R. Michel, J. Echevarria, T. Cang +2

ROTSE1 J164341.65+251748.1 was photometrically observed in the V band during three epochs with the 0.84-m telescope of the San Pedro Mártir Observatory in Mexico. Based on addition…

astro-ph.SR2012

Solar like oscillations in the stars KIC 5390438 and KIC 5701829 observed by Kepler

L. Fox-Machado, A. S. Baran

The preliminary results of an analysis of the KIC 5390438 and KIC 5701829 light curves are presented. The variations of these stars were detected by Baran et al. (2011a) in a searc…

astro-ph.SR20111 cited

Asterosesimology of the Delta Scuti Star V650 Tauri

L. Fox-Machado, R. Michel, M. Alvarez +2

The preliminary results of a multisite photometric campaign on the Pleiades Delta Scuti variable V650 Tauri are reported. The star was observed photometrically for 14 days during 2…