2 edition of open clusters NGC 2533, NGC 2567, NGC 2571, and Ru 58. found in the catalog.
open clusters NGC 2533, NGC 2567, NGC 2571, and Ru 58.
Bibliography: p. 604.
|Series||Arkiv för astronomi,, bd. 4, nr. 39|
|LC Classifications||QB1 .A293 bd. 4, nr. 39|
|The Physical Object|
|Number of Pages||611|
|LC Control Number||70403027|
NGC (also catalogued as NGC ) is an open cluster in the constellation was discovered by William Herschel on December 9, The cluster was also observed by John Herschel on January 7, He also observed it on February 5, , identifying it as a different object, which was catalogued as NGC 1. Introduction. The rich galactic open star cluster NGC , in the constellation of Puppis (α = 08 h 00 m 48 s, δ = − 19 ∘ 03 ′ 06 ″) is at a distance of ± 15 age of this cluster is estimated to be ∼ 8 × 10 9 years and is thought to be older than M 67, but younger than NGC (Sujatha and Babu, ).Ensemble photometry of stars, constant as well as.
European astronomers have performed a comprehensive study of the young open cluster NGC The new research resulted in determining fundamental parameters of dozens of stars in the cluster and. In this week's Astronomy magazine podcast, we'll help you observe open clusters NGC and NGC , barred spiral galaxy NGC , and emission nebula Sharpless 2– in your winter night sky.
NGC , NGC , and Sextans A (kB) Oh, my aching heart This week’s small-telescope target is the Heart and Dagger Cluster, also known as open cluster NGC in Puppis. Cluster in NGC Stephen Skinner CASA, Univ. of Colorado, Boulder, CO Marc Gagn´e and Emily Belzer Dept. of Geology & Astronomy, West Chester Univ., West Chester, PA ABSTRACT We present results of a sensitive 76 ksec Chandra observation of the young stellar cluster in NGC , lying at a distance of ∼ pc in the.
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Journal Article: THE OPEN CLUSTER NGCNGCNGCAND Ru The open clusters NGCNGCNGCand Ru 58Author: U. Lindoff. Title: The open clusters NGCNGCNGCand Ru 58 Authors: Lindoff, U. Journal: Ark. Astr. Vol. 4, p Bibliographic Code: ArAL. Complete bibliographic record Other article options Print this article; Previous article page Print this page Next article page.
NGC (also known as the Owl Cluster, the ET Cluster, or Caldwell 13) is an open star cluster in the constellation was discovered by William Herschel inand lies over 7, light years away from the has an estimated age of 21 million years.
The cluster is sometimes referred by amateur astronomers as the Owl Cluster, Kachina Doll Cluster, the ET Cluster (due to its Constellation: Cassiopeia. of NGCNGCKoposov 53 and Be 89 are displayed in Figure 1.
NGC The southern young open cluster NGC is a moderate young open clus-ter located in low absorption region associated with Vela Puppis (Giorgi et al., ) and projected in Author: Ferhat F. Özeren, Özgün Arslan, İbrahim Küçük, İnci Akkaya Oralhan. This image contains six open clusters -- K Harv Frolov 1, NGCNGCand Berkeley 58 -- and one emission nebula -- Sh All of the clusters except Frolov and Ru 58.
book are on a nearly straight line starting with King 12 at the top right and ending with Berkeley 58 near the left edge, about one-third of the field up from the bottom.
Analysing the database for stars in open clusters I. General methods and description of the data Be 62 Ho 10 24 NGC NGC NGC Ru 18 Be 69 Ho 16 86 NGC. An older and more compact open cluster, NGCis at the lower right. NGC is four times more distant than M35, over 10 times older, and much more compact with many more stars in roughly the same volume of space.
NGC 's bright blue stars have self-destructed, leaving cluster light to be dominated by older and yellower stars. The existence and relationship of the possible clusters NGCNGC and NGC has been a matter of discussion during the last decades.
This star field is close to the galactic anticenter and lies in the direction of the Taurus dark cloud complex. As part of a comprehensive astrometric and photometric analysis of this zone, we present a brief historical introduction together with deep. The overlapping open clusters NGC and NGC II.
Section 3 is devoted to the photometric calibration of the plates, and includes a brief discussion of the resulting stan-dard BVR photographic photometry. The iterative cen-tral overlap algorithm is described in Sect.
Section 5. in the ﬁeld of the northern open cluster NGC, for which little information is available. We provide also BV CCD photometry of a ﬁeld 5′ northward of NGC to take into account ﬁeld star contamination.
We argue that NGC is a young compact open cluster, for which we estimate a core radius in the range − arcmin. The open clusters NGCNGCNGCand Ru Article. Jan ; U. Lindoff; View. On the problem of distribution in globular clusters. In this paper, we analyze the open cluster. The open cluster NGC Home Your Sky Constellations List Puppis NGC News °58' Sources  OpenNGC (Mattia Verga)  The Collinder Catalog of Open Star Clusters: Visibility from Redmond.
All times shown in Redmond local time. Events. 16 Jan Open Clusters 7 Open Cluster Observing Log (1) Object Date Object Date Berk 58 NGC Berk 59 DODZ 3 King 13 Cr 69 Berk 2 NGC King 14 DODZ 4 NGC NGC King 16 NGC NGC NGC NGC NGC Tr 1 NGC Cr Ru 1 Stock 4 Ru 3. open clusters NGC and NGC (V(I)C and UBV(RI)C respectively).
From the analysis of our data we found that NGC is located at a distance of about 4 kpc and its age is close to Myr. As for NGCit is placed at about 5 kpc from the Sun and is Myr old.
This means that NGC belongs to the extension. The young open star cluster NGC (C) has been neglected, mostly because it ap-pears in a crowded eld only four degrees from the Galactic center (see Fig. The most recent study of the cluster, by Carraro et al. (), de-rived an age of 50 Myr (million years) and distance of kpc.
These authors noted that the nearby. The Double Cluster, or Caldw is the name for two open clusters – NGC and NGC – located close together in Perseus known as h Persei and χ Persei (h and Chi Persei), the clusters both lie at an approximate distance of 7, light years from Earth and are.
Both clusters are extremely young and spatially close to each other. It's estimated that NGC is million years old and NGC is million years old. For comparison, the Pleiades (M45) open cluster is million years old. In total, NGC and NGC contain at least hot blue-white supermassive and super luminous giant stars.
Category:NGC open clusters. From Wikimedia Commons, the free media repository. Jump to navigation Jump to search. NGC (3 F) NGC (3 F) NGC (3 F) NGC (1 F) NGC (3 F) NGC.
The open cluster NGC Red-band image from the Second Digitized Sky Survey (DSS2), measuring 10 arcminutes across. Finder chart. Please wait Loading 0 /4 Click and drag to rotate Mouse wheel to zoom in/out Touch with mouse to dismiss Click and drag the chart above to pan around the sky, or use the mouse wheel to zoom.
Based on 2MASS J and Ks photometry for the open star clusters NGCNGCPismis 6, Pismis 8 and using color magnitude diagrams with isochrones ﬁt, we found an age of log(age) = ( ± 6 Myr) for NGC and log(age) = (8 ± 6 Myr) for NGC For Pismis 6 and Pismis 8 we adopted a range of log(age) = 6 - 7 (1 - 10 Myr).OPEN CLUSTERS.
Glittering stars of many colours sprinkled across the view. Some bright, some not so bright, some appear as a rich grouping of jewels on a velvet background, while others are just a sparse scattering of faint lights. NGC NGC NGC The Jewel Box Cluster: NGC NGC NGC NGC NGC NGC The Globular Cluster Systems of NGC and NGC in the Antlia Cluster ⋆ B.
Dirsch1, T. Richtler1, L.P. Bassino2 1 Universidad de Concepcio´n, Departamento de F´ısica, Casilla C, Concepcio´n, Chile 2 Facultad de Ciencias Astrono´micas y Geof´ısicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, La Plata.