scholarly journals Eclipsing Binaries in the Open Cluster Ruprecht 147. IV: The Active Triple System EPIC 219511354

2021 ◽  
Vol 921 (2) ◽  
pp. 133
Author(s):  
Guillermo Torres ◽  
Andrew Vanderburg ◽  
Jason L. Curtis ◽  
Adam L. Kraus ◽  
Eric Gaidos
2020 ◽  
Vol 896 (2) ◽  
pp. 162 ◽  
Author(s):  
Guillermo Torres ◽  
Andrew Vanderburg ◽  
Jason L. Curtis ◽  
Adam L. Kraus ◽  
Aaron C. Rizzuto ◽  
...  

2001 ◽  
Vol 375 (2) ◽  
pp. 375-386 ◽  
Author(s):  
M. van den Berg ◽  
J. Orosz ◽  
F. Verbunt ◽  
K. Stassun

2005 ◽  
Vol 277-279 ◽  
pp. 869-875
Author(s):  
Hwihyun Kim ◽  
Yong Ik Byun

We present the result of photometric variability investigation for stars in the field of M67. The old open cluster M67, one of the most studied open clusters, shows the sign of significant main-sequence binary population in its color-magnitude diagrams. Identification of eclipsing binaries and follow-up studies will enable us to study the nature of binary population in most direct manner. We used approximately 350 images from the BATC (Beijing-Arizona-Taipei-Connecticut) data archive to examine variability within one square degree field centered on M67. A total of 18 stars were classified to be real variables. Our new discoveries include seven eclipsing binary systems of which two are likely to be W UMa systems. All of these variables were found using the phase dispersion minimization (PDM) method developed by Shin and Byun[11].


2019 ◽  
Vol 487 (3) ◽  
pp. 3505-3522 ◽  
Author(s):  
Gabriela Michalska

ABSTRACT We present results of a UBVIC variability survey in the young open cluster NGC 2244. In total, we found 245 variable stars. Most of them, 211 stars, are variables with irregular variations. Furthermore, 23 periodic variables were found. We also detected four candidates for δ Scuti stars and seven eclipsing binaries. Based on the mid-infrared Spitzer and WISE photometry and near infrared JHKS 2MASS photometry, we classified 104 young stellar sources among our variables: 1 Class I object, 1 Class I/flat spectrum object, 4 flat spectrum objects, 91 Class II objects, and 7 transition disc objects. This classification, together with r′i′Hα IPHAS photometry and JHK UKIDSS photometry, were used for identification of pre-main sequence stars among irregular and periodic variables. In this way, 97 CTTS candidates (96 irregular and one periodic variable), 68 WTTS candidates (54 irregular and 14 periodic variables), and 6 Herbig Ae/Be stars were found. For 223 variable stars we calculated membership probability based on proper motions from Gaia DR2 catalogue. Majority of them, 143 stars, are cluster members with probability greater than 70 per cent. For only 36 variable stars the membership probability is smaller than 20 per cent.


2006 ◽  
Vol 2 (S240) ◽  
pp. 619-621
Author(s):  
John Southworth

AbstractDetached eclipsing binaries are very useful objects for calibrating theoretical stellar models and checking their predictions. Detached eclipsing binaries in open clusters are particularly important because of the additional constraints on their age and chemical composition from their membership of the cluster. I compile a list containing absolute parameters of well-studied eclipsing binaries in open clusters, and present new observational data on the B-type systems V1481 Cyg and V2263 Cyg which are members of the young open cluster NGC 7128.


1993 ◽  
Vol 262 (1) ◽  
pp. 49-56 ◽  
Author(s):  
Janusz Kaluzny ◽  
Beata Mazur ◽  
Wojciech Krzeminski

2013 ◽  
Vol 13 (9) ◽  
pp. 1052-1062 ◽  
Author(s):  
Xiang-Song Fang ◽  
Sheng-Hong Gu ◽  
Li-Yun Zhang ◽  
Qing-Feng Pi

2019 ◽  
Vol 485 (2) ◽  
pp. 2562-2572 ◽  
Author(s):  
T Hajdu ◽  
T Borkovits ◽  
E Forgács-Dajka ◽  
J Sztakovics ◽  
G Marschalkó ◽  
...  

2019 ◽  
Vol 82 ◽  
pp. 99-106 ◽  
Author(s):  
T. Borkovits ◽  
E. Forgács-Dajka ◽  
S.A. Rappaport

Tidally forced apsidal motion in eccentric eclipsing binaries is a key observable of stellar structure studies, and may serve as important probe for different tidal dissipation theories. There are, however, alternative physical processes which result in additional contributions to the observed apsidal motion. Here we mainly concentrate on the perturbing effect of a third, distant stellar companion, forming a hierarchical triple system with the eclipsing pair. First we discuss the mathematical form of the combined third body and tidally forced apsidal motions, and its observational aspects. Then we present a brief description of an eclipse timing variation study (based on the above mentioned analytical formulae) of 26 Kepler spacecraft-discovered 3-rd body perturbation-dominated compact hierarchical triples.


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