activity
20042026
most citedThe shortest period M-dwarf eclipsing system BW3 V38, II: determination of absolute elements

53 citations · 154 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

A short-period binary OGLE-BLG-ELL-006503 showing slow variations in brightness

S. M. Rucinski

Analysis of 28 years of OGLE project data for the 0.404 day period binary OGLE BLG ELL-006503 (V1231 Sco) shows a superposition of tidal-interaction variations of about 0.07 magnit…

astro-ph.SR2021★ 31 cited

Physical parameters of close binary systems: VIII

K. Gazeas, S. Zola, A. Liakos +13

This paper presents the results of a combined spectroscopic and photometric study of 20 contact binary systems: HV Aqr, OO Aql, FI Boo, TX Cnc, OT Cnc, EE Cet, RWCom, KR Com, V401…

astro-ph.SR2013★ 1 cited

The Clusters AgeS Experiment (CASE): The blue straggler Star M55-V60 caught amidst rapid mass exchange

M. Rozyczka, J. Kaluzny, I. B. Thompson +3

We analyze light and velocity curves of the eclipsing blue straggler V60 in the field of the globular cluster M55. We derive Mp=1.259+-0.025 Msun, Rp=1.102+-0.021 Rsun, Mbol,p=3.03…

astro-ph.SR2013★ 11 cited

mu Eridani from MOST and from the ground: an orbit, the SPB component's fundamental parameters, and the SPB frequencies

M. Jerzykiewicz, H. Lehmann, E. Niemczura +15

MOST time-series photometry of mu Eri, an SB1 eclipsing binary with a rapidly-rotating SPB primary, is reported and analyzed. The analysis yields a number of sinusoidal terms, main…

astro-ph.SR2011

Photometric study of the star cluster NGC 2155 in the Large Magellanic Cloud: age estimation and variable stars

M. Otulakowska, A. Olech, W. Pych +3

We present results of new photometry for the globular star cluster NGC 2155 in the Large Magellanic Cloud (LMC). Our I- and V-band observations were obtained with the 6.5-meter Mag…

astro-ph.SR2009★ 6 cited

Physical parameters of components in close binary systems: V

S. Zola, J. M. Kreiner, B. Zakrzewski +9

The paper presents combined spectroscopic and photometric orbital solutions for ten close binary systems: CN And, V776 Cas, FU Dra, UV Lyn, BB Peg, V592 Per, OU Ser, EQ Tau, HN UMa…