Search results for "Open star clusters"

showing 10 items of 27 documents

Chandra X-ray sources in Orion Nebula Cluster

2003

In this first of two companion papers on the Orion Nebula Cluster (ONC), we present our analysis of a 63ks Chandra HRC-I observation that yielded 742 X-ray detections within the 30'x30' field of view. To facilitate our interpretation of the X-ray image, here we collect a multiwavelength catalog of nearly 2900 known objects in the region by combining 17 different catalogs from the recent literature. We define two reference groups: an infrared sample, containing all objects detected in the K band, and an optical sample comprising low-extinction, well-characterized ONC members. We show for both samples that field object contamination is generally low. Our X-ray sources are primarily low-mass O…

Open star clustersAstrophysics and AstronomyX ray sourcesStellar AstronomyPhysicsNatural SciencesX-ray sourcescosmology
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X-ray Luminosities in Blanco 1

2005

We present X-ray Luminosity Distributions (XLDs) of late-type members (dF, dG, dK, dM) of the Blanco 1 cluster, based on ROSAT-HRI data and new astrometric-photometric membership obtained from the GSC-II project. For the first time we present the XLD of dM stars of this cluster. The high metallicity of Blanco 1 allows us to investigate the role of chemical composition on the coronal emission of late-type stars. Comparison between X-ray Luminosity Distributions of Blanco 1 and Pleiades, NGC 2516 and {alpha} Per suggests a possible metallicity effect in dM stars. Cone search capability for table J/A+A/399/919/tablea1 (Optical, infrared and X-ray band properties of Blanco 1 members in the comb…

Open star clustersAstrophysics and AstronomyX ray sourcesStellar AstronomyPhysicsNatural SciencesX-ray sourcescosmology
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BVI photometry in NGC 6611

2007

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Correlation between the spatial distribution of circumstellar disks and massive stars in the open cluster NGC 6611. Compiled catalog and cluster parameters.' (bibcode: 2007A&A...462..245G)

Open star clustersPhotometryAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsWide-band photometryAstrophysics::Galaxy AstrophysicsInfrared photometryOptical astronomy
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BVI & JHK photometry of NGC 3960

2004

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Parameter properties and stellar population of the old open cluster NGC 3960.' (bibcode: 2004A&A...417..945P)

Open star clustersPhotometryCCD photometryWide-band photometryInfrared photometryOptical astronomy
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Mapping accretion variability in NGC 2264

2014

Our study aims at characterizing the accretion properties of several hundred members of the star-forming region NGC 2264 (3Myr). We performed a deep u,g,r,i mapping of the cluster with CFHT/MegaCam, and monitored the simultaneous u+r variability of its members over a baseline of two weeks. Stellar parameters are determined homogeneously for about 750 monitored young objects, 40% of which are accreting T Tauri stars. Accretion properties and accretion variability are investigated and characterized from UV excess measurements. Non-accreting members of the cluster define the reference UV emission level over which flux excess is detected and measured. Cone search capability for table J/A+A/570/…

Open star clustersPhotometryobservational astronomyAccretionAstrophysics and AstronomyPhysicsCCD photometryAstrophysical ProcessesNatural SciencesSloan photometrystellar astronomyOptical astronomy
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X-ray sources in NGC 752

2008

While observational evidence shows that most of the decline in a star's X-ray activity occurs between the age of the Hyades (~8x10^8yr) and that of the Sun, very little is known about the evolution of stellar activity between these ages. To gain information on the typical level of coronal activity at a star's intermediate age, we studied the X-ray emission from stars in the 1.9Gyr old open cluster NGC 752. We analysed a ~140ks Chandraobservation of NGC 752 and a ~50ks XMM-Newtonobservation of the same cluster. We detected 262 X-ray sources in the Chandra data and 145 sources in the XMM-Newton observation. Around 90% of the catalogued cluster members within Chandra's field-of-view are detect…

Open star clustersPhotometryobservational astronomyAstrophysics and AstronomyX ray sourcesStellar AstronomyPhysicsX-ray sourcesNatural SciencescosmologyInfrared photometry
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PMS stars in h Per

2016

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Supersaturation and activity-rotation relation in PMS stars: the young cluster h Per.' (bibcode: 2016A&A...589A.113A)

Open star clustersPre-main sequence starsX-ray sources
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XMM survey of NGC 2516

2007

VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Deep X-ray survey of the young open cluster NGC 2516 with XMM-Newton.' (bibcode: 2006A&A...450..993P)

Open star clustersX-ray sources
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Gamma Vel cluster membership and IMF

2016

Understanding the properties of young open clusters, such as the Initial Mass Function (IMF), star formation history and dynamic evolution, is crucial to obtain reliable theoretical predictions of the mechanisms involved in the star formation process. We want to obtain a list, as complete as possible, of confirmed members of the young open cluster Gamma Velorum, with the aim of deriving general cluster properties such as the IMF. We used all available spectroscopic membership indicators within the Gaia-ESO public archive together with literature photometry and X-ray data and, for each method, we derived the most complete list of candidate cluster members. Then, we considered photometry, gra…

Open star clustersobservational astronomyPre main sequence starsRadial velocityAstrophysics and AstronomyHertzsprung Russell diagramPhysicsexoplanet astronomyStellar massesPre-main sequence starsNatural Sciencesstellar astronomySpectroscopy
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GES: pre-main-sequence clusters [Fe/H]

2017

The radial metallicity distribution in the Galactic thin disc represents a crucial constraint for modelling disc formation and evolution. Open clusters allow us to derive both the radial metallicity distribution and its evolution over time. In this paper we perform the first investigation of the present-day radial metallicity distribution based on [Fe/H] determinations in late type members of pre-main-sequence clusters. Because of their youth, these clusters are therefore essential for tracing the current inter-stellar medium metallicity. We used the products of the Gaia-ESO Survey analysis of 12 young regions (age<100Myr), covering Galactocentric distances from 6.67 to 8.70kpc. For the fir…

galactic and extragalactic astronomyAstrophysics and AstronomyPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsChemical abundancesAstrophysics::Cosmology and Extragalactic AstrophysicsMilky Way Galaxystellar astronomyInterdisciplinary AstronomyEffective temperatureOpen star clustersobservational astronomyAstrophysics::Earth and Planetary AstrophysicsNatural SciencesAstrophysics::Galaxy Astrophysics
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