scholarly journals An observational asteroseismic study of the pulsating B-type stars in the open cluster NGC 884

2013 ◽  
Vol 9 (S301) ◽  
pp. 479-480
Author(s):  
S. Saesen ◽  
M. Briquet ◽  
C. Aerts ◽  
A. Miglio ◽  
F. Carrier
Keyword(s):  
Chemical Composition ◽  
Recent Progress ◽  
Massive Stars ◽  
Open Cluster ◽  
Seismic Interpretation ◽  
Evolution Model ◽  
Stellar Structure ◽  
Current Status ◽  
Physical Description ◽  
Young Open Cluster

AbstractRecent progress in the seismic interpretation of field β Cep stars has resulted in improvements of the physical description in the stellar structure and evolution model computations of massive stars. Further asteroseismic constraints can be obtained from studying ensembles of stars in a young open cluster, which all have similar age, distance and chemical composition. We present an observational asteroseismic study based on the discovery of numerous multi-periodic and mono-periodic B-type stars in the open cluster NGC 884 (χ Persei). Our study illustrates the current status of ensemble asteroseismology of this young open cluster.

scholarly journals NGC 3293 revisited by the Gaia-ESO Survey

2014 ◽  
Vol 9 (S307) ◽  
pp. 140-141
Author(s):  
Thierry Semaan ◽  
Thierry Morel ◽  
Eric Gosset ◽  
Juan Zorec ◽  
Yves Frémat ◽  
...  
Keyword(s):  
Massive Stars ◽  
Open Cluster ◽  
Second Step ◽  
Chemical Abundances ◽  
Hot Stars ◽  
Fundamental Parameters ◽  
Medium Resolution ◽  
Young Open Cluster ◽  
Extended View

AbstractIn the framework of the Gaia-ESO survey we have determined the fundamental parameters of a large number of B-type stars in the Galactic, young open cluster NGC 3293. The determination of the stellar parameters is based on medium-resolution spectra obtained with FLAMES/GIRAFFE at ESO-VLT. As a second step, we adopted the accurate parameters to determine the chemical abundances of these hot stars. We present a comparison of our results with those obtained by the 'VLT-FLAMES survey of massive stars' (Evans et al. 2005). Our study increases the number of objects analysed and provides an extended view of this cluster.

scholarly journals Eclipsing Binaries in Open Clusters

2006 ◽  
Vol 2 (S240) ◽  
pp. 619-621
Author(s):  
John Southworth
Keyword(s):  
Chemical Composition ◽  
Observational Data ◽  
Open Cluster ◽  
Type Systems ◽  
Open Clusters ◽  
Eclipsing Binaries ◽  
Young Open Cluster ◽  
Stellar Models ◽  
Additional Constraints ◽  
Absolute Parameters

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.

scholarly journals Correlation between the spatial distribution of circumstellar disks and massive stars in the young open cluster NGC 6611

2009 ◽  
Vol 496 (2) ◽  
pp. 453-463 ◽  
Author(s):  
M. G. Guarcello ◽  
G. Micela ◽  
F. Damiani ◽  
G. Peres ◽  
L. Prisinzano ◽  
...  
Keyword(s):  
Spatial Distribution ◽  
Massive Stars ◽  
Open Cluster ◽  
Circumstellar Disks ◽  
Young Open Cluster

scholarly journals Recent progress in materials development for CO2 conversion: issues and challenges

2021 ◽  
Author(s):  
Sourav Ghosh ◽  
Arindam Modak ◽  
Arnab Samanta ◽  
Kanika Kole ◽  
Subhra Jana
Keyword(s):  
Recent Progress ◽  
Value Added ◽  
Advanced Materials ◽  
Current Status ◽  
Co2 Conversion ◽  
Technical Feasibility ◽  
Materials Development

A comprehensive and critical in-depth discussion on the development and prospect of several advanced materials for conversion of CO2 to value added chemicals is provided, together with their current status, technical feasibility and future opportunities.

scholarly journals [ITAL]UBVRI[/ITAL] and Hα Photometry of the Young Open Cluster NGC 6530

2000 ◽  
Vol 120 (1) ◽  
pp. 333-348 ◽  
Author(s):  
Hwankyung Sung ◽  
Moo-Young Chun ◽  
Michael S. Bessell
Keyword(s):  
Open Cluster ◽  
Young Open Cluster

scholarly journals ASPITZERVIEW OF THE YOUNG OPEN CLUSTER NGC 2264

2009 ◽  
Vol 138 (4) ◽  
pp. 1116-1136 ◽  
Author(s):  
Hwankyung Sung ◽  
John R. Stauffer ◽  
Michael S. Bessell
Keyword(s):  
Open Cluster ◽  
Young Open Cluster

scholarly journals CHARACTERIZATION OF THE YOUNG OPEN CLUSTER G144.9+0.4 IN THE CAMELOPARDALIS OB1 ASSOCIATION

2013 ◽  
Vol 775 (2) ◽  
pp. 123
Author(s):  
Chien-Cheng Lin ◽  
W. P. Chen ◽  
Neelam Panwar
Keyword(s):  
Open Cluster ◽  
Young Open Cluster

scholarly journals The young open cluster Trumpler 3

2010 ◽  
Vol 331 (3) ◽  
pp. 312-322
Author(s):  
G. Maciejewski ◽  
L. Bukowiecki
Keyword(s):  
Open Cluster ◽  
Young Open Cluster

scholarly journals Defining the Binary Star Population in the Young Open Cluster M35 (NGC 2168)

2007 ◽  
Vol 3 (S246) ◽  
pp. 105-106
Author(s):  
Ella K. Braden ◽  
Robert D. Mathieu ◽  
Sören Meibom
Keyword(s):  
Binary Systems ◽  
Initial Conditions ◽  
Binary Star ◽  
Open Cluster ◽  
Open Clusters ◽  
Spatial Period ◽  
Large Sample Size ◽  
Long Baseline ◽  
Dynamical Simulations ◽  
Young Open Cluster

AbstractWe present current results from the ongoing WIYN Open Cluster Study radial-velocity survey for 1410 stars in the young (150 Myr) open cluster M35 (NGC 2168) and establish a benchmark for initial conditions in young open clusters. We find for periods ≲ 1000 days a minimum binary frequency of 0.36 – 0.51. We also analyze the spatial, period and eccentricity distributions of the binary systems and find that the period and eccentricity distributions are well approximated by scaled field distributions from Duquennoy & Mayor (1991). With our large sample size and long baseline, we have a unique understanding of the binary population in this young cluster, making it ideal for defining initial conditions for dynamical simulations.

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