activity
20052024
most citedHow stellar activity affects the size estimates of extrasolar planets

155 citations · 795 across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.SR2024★ 20 cited

Prominence activation, optical flare, and post-flare loops on the RS Canum Venaticorum star SZ Piscium

Dongtao Cao, Shenghong Gu, Jian Ge +7

We present the results of time-resolved high-resolution spectroscopic observations of the very active RS Canum Venaticorum (RS CVn) star SZ Piscium (SZ Psc), obtained during two co…

astro-ph.SR2024★ 7 cited

Prominence detection and chromosphere feature on the prototype RS CVn of active binary systems

Dongtao Cao, Shenghong Gu, U. Wolter +4

We present a study of high-resolution spectra of RS Canum Venaticorum (RS CVn), a prototype of active binary systems. Our data were obtained from 1998 to 2017 using different teles…

astro-ph.SR2020★ 4 cited

Time series of optical spectra of Nova V659 Sct

Dennis Jack, Klaus-Peter Schröder, Philippe Eenens +4

With our robotic 1.2 m TIGRE telescope, we were able to obtain eight optical spectra with intermediate resolution (R = 20,000) of the Nova V659 Sct during different phases of its o…

astro-ph.SR2020★ 54 cited

An X-ray activity cycle on the young solar-like star

M. Coffaro, B. Stelzer, S. Orlando +7

In 2015 we started the XMM-Newton monitoring of the young solar-like star Epsilon Eridani (440 Myr), one of the youngest solar-like stars with a known chromospheric CaII cycle. By…

astro-ph.SR2020★ 12 cited

The first Doppler imaging of the active binary prototype RS Canum Venaticorum

Yue Xiang, Shenghong Gu, U. Wolter +6

We present the first Doppler images of the prototypical active binary star RS CVn, derived from high-resolution spectra observed in 2004, 2016 and 2017, using three different teles…

astro-ph.SR2019★ 2 cited

An eccentric wave in the circumstellar disc of the Be/X-ray binary X Persei

R. K. Zamanov, K. A. Stoyanov, U. Wolter +7

We present spectroscopic observations of the Be/X-ray binary X Per obtained during the period December 2017 - January 2020 (MJD~58095 - MJD~58865). In December 2017 the , ,…