Open cluster king 10
Web1 de jan. de 1992 · CCD photometry of the open cluster King 10 has been carried out in the UBVRI photometric passbands down to V of about 19.5 mag. The reddening for the cluster region is found to be variable. WebDA page for open cluster King 5. Basic Parameters: DSS Image: 10 x 10 arcminutes; Right Ascension (2000) 03 14 45: Declination (2000) +52 41 12: Galactic longitude: …
Open cluster king 10
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Web2MASS NEAR-IR CMD OF THE OPEN CLUSTER KING 11 35 (Nikolaev et al. 2000). This paper is arranged as follows. Section 2 de-scribes the near-IR CMD of King 11. In … WebThe best fit to the radial surface bright- ness profile with a single-mass King's model (Figure 3) ... (Ivanov et al. 2005) but this is however not the case, in general, for open clusters.
Web18 de mai. de 2024 · The finding charts for the clusters IC 1442, King 21, and Tr 7. The image sizes are 180 180. age open clusters (Joshi et al.2012,2014,2024;Maurya & Joshi 2024). In this paper, we present a comprehensive photometric study of three young open clusters IC 1442, King 21, and Tr 7 as contin-uation of our ongoing project of … WebPhotoelectric magnitudes of 30 stars in the field of King 12 have been obtained. The reddening is variable across the cluster. A distance of 2.49 kiloparsecs has been …
Webcolour–magnitude diagram of King 1 with those of similar open clusters and with different setsofisochrones,wehaveestimatedanageof2.8±0.3Gyr,adistancemodulusof(m−M) o =10.6±0.1magandareddeningofE(B−V)=0.80±0.05mag.Tocompleteouranalysis, we acquired medium resolution spectra for 189 stars in the area of King 1. From their derived WebDA page for open cluster King 2. Basic Parameters: DSS Image: 10 x 10 arcminutes; Right Ascension (2000) 00 51 00: Declination (2000) +58 11 00: Galactic longitude: …
WebDA page for open cluster King 2. Basic Parameters: DSS Image: 10 x 10 arcminutes; Right Ascension (2000) 00 51 00: Declination (2000) +58 11 00: Galactic longitude: 122.874: Galactic latitude ... From cluster chart (plotted) The cross-reference table; The Budapest bibliography (Alter et al.)
Web17 de dez. de 2009 · The target clusters have been selected on the basis of the following criteria. A high Galactic latitude (b > 15°) in order to limit the field contamination. An absolute visual magnitude M V < −2.5 in order to detect a significant sample of cluster stars. Five cluster passed these criteria namely NGC 188, 2204, 2243, 2420 and 2516. cult witchWebWe have obtained CCD BVI imaging of the old open clusters Berkeley 32 and King 11. Using the synthetic colour-magnitude diagram method with three different sets of stellar evolution models of various metallicities, with and without overshooting, we have determined their age, distance, reddening, and indicative metallicity, as well as distance from the … cult wing leedsWebDA page for open cluster King 19. Basic Parameters: DSS Image: 10 x 10 arcminutes; Right Ascension (2000) 23 08 18: Declination (2000) +60 31 00: Galactic longitude: ... From cluster map (scanned) From cluster chart (plotted) The cross-reference table; The Budapest bibliography (Alter et al.) cult wines logoWeb15 de abr. de 2024 · Homes similar to 6623 Mccambell Cluster are listed between $1M to $1M at an average of $430 per square foot. OPEN SAT, 2PM TO 4PM. $1,389,000. 6 … east molesey roofing gutteringWebThe meaning of OPEN CLUSTER is a cluster of stars in which all the individual members may be discerned with an optical aid and which is much less compact and has fewer … cult wines of napaWeb30 de mai. de 2024 · We present a CCD photometric survey for the search of variable stars in four open clusters namely Berkeley 69, King 5, King 7 and Berkeley 20. The time series observations were carried out for 1 and/or 2 nights for each of the clusters in the year 1998, which have led to identify nineteen variable stars in these clusters. Out of these 19 … cultwo blockbWeb15 de jan. de 2016 · Surface and spatial radial density profiles in open clusters are derived using a kernel estimator method. Formulae are obtained for the contribution of every star into the spatial density profile. The evaluation of spatial density profiles is tested against open-cluster models from N-body experiments with N = 500. Surface density profiles … cult with purple blankets