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NGC 6553

NGC 6553 is a globular cluster in the constellation Sagittarius. NGC 6553 has an apparent magnitude of about 8th magnitude with an apparent diameter of 8.2 arcminutes.[2] Its Shapley–Sawyer Concentration Class is XI,[2] meaning the star concentration is very loose even at the center; it has stars of magnitude 20 and dimmer. It is located just over a degree southeast of Messier 8, the Lagoon Nebula.

NGC 6553
The globular cluster NGC 6553 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ClassV
ConstellationSagittarius
Right ascension18h 09m 15.68s[1]
Declination−25° 54′ 27.9″[1]
Distance19.6 kly
(6.01 kpc)[1]
Apparent magnitude (V)8.06[2]
Physical characteristics
Radius4.1' x 4.1'[2]
Metallicity = -0.18[3] dex
Other designationsGCl 88, C 1806-259[1]
See also: Globular cluster, List of globular clusters

Unlike common globular clusters, NGC 6553 is relatively metal-rich, and there is evidence of at least two periods of star formation.[4] Due to a complex star-forming record, the stars in the cluster are differing in composition, most notably in concentrations of sodium and aluminium.[5]

NGC 6553 is very similar in composition to NGC 6528, suggesting an origin in a similar environment.[6]

References

  1. ^ a b c d "NGC 6553". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 January 2017.
  2. ^ a b c d "NGC 6553". Retrieved 8 January 2016.
  3. ^ "A Galactic Globular Clusters Database: NGC 6553". Retrieved 8 January 2017.
  4. ^ Tang, Baitian; Cohen, Roger E.; Geisler, Doug; Schiavon, Ricardo P.; Majewski, Steven R.; Villanova, Sandro; Carrera, Ricardo; Zamora, Olga; Garcia-Hernandez, D. A.; Shetrone, Matthew; Frinchaboy, Peter; Meza, Andres; Fernández-Trincado, J. G.; Muñoz, Ricardo R.; Lin, Chien-Cheng; Lane, Richard R.; Nitschelm, Christian; Pan, Kaike; Bizyaev, Dmitry; Oravetz, Daniel; Simmons, Audrey (2016), "Two groups of red giants with distinct chemical abundances in the bulge globular cluster NGC 6553 through the eyes of APOGEE", Monthly Notices of the Royal Astronomical Society, 465: 19–31, arXiv:1610.06763, doi:10.1093/mnras/stw2739
  5. ^ Muñoz, C.; Villanova, S.; Geisler, D.; Cortés, C. C.; Moni Bidin, C.; Cohen, R. E.; Saviane, I.; Dias, B.; Tang, B.; Mauro, F. (2019), "The vertical Na–O relation in the bulge globular cluster NGC 6553", Monthly Notices of the Royal Astronomical Society, 492 (3): 3742–3752, arXiv:1912.03742, doi:10.1093/mnras/stz3586
  6. ^ Muñoz, C.; Geisler, D.; Villanova, S.; Saviane, I.; Cortés, C. C.; Dias, B.; Cohen, R. E.; Mauro, F.; Moni Bidin, C. (2018), "Chemical analysis of NGC 6528: One of the most metal-rich bulge globular clusters", Astronomy & Astrophysics, 620: A96, arXiv:1809.04164, doi:10.1051/0004-6361/201833373, S2CID 119085692

External links

  •   Media related to NGC 6553 at Wikimedia Commons
  • NGC 6553


6553, globular, cluster, constellation, sagittarius, apparent, magnitude, about, magnitude, with, apparent, diameter, arcminutes, shapley, sawyer, concentration, class, meaning, star, concentration, very, loose, even, center, stars, magnitude, dimmer, located,. NGC 6553 is a globular cluster in the constellation Sagittarius NGC 6553 has an apparent magnitude of about 8th magnitude with an apparent diameter of 8 2 arcminutes 2 Its Shapley Sawyer Concentration Class is XI 2 meaning the star concentration is very loose even at the center it has stars of magnitude 20 and dimmer It is located just over a degree southeast of Messier 8 the Lagoon Nebula NGC 6553The globular cluster NGC 6553 imaged by the Hubble Space TelescopeObservation data J2000 epoch ClassVConstellationSagittariusRight ascension18h 09m 15 68s 1 Declination 25 54 27 9 1 Distance19 6 kly 6 01 kpc 1 Apparent magnitude V 8 06 2 Physical characteristicsRadius4 1 x 4 1 2 Metallicity Fe H displaystyle begin smallmatrix left ce Fe ce H right end smallmatrix 0 18 3 dexOther designationsGCl 88 C 1806 259 1 See also Globular cluster List of globular clustersUnlike common globular clusters NGC 6553 is relatively metal rich and there is evidence of at least two periods of star formation 4 Due to a complex star forming record the stars in the cluster are differing in composition most notably in concentrations of sodium and aluminium 5 NGC 6553 is very similar in composition to NGC 6528 suggesting an origin in a similar environment 6 References Edit a b c d NGC 6553 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 8 January 2017 a b c d NGC 6553 Retrieved 8 January 2016 A Galactic Globular Clusters Database NGC 6553 Retrieved 8 January 2017 Tang Baitian Cohen Roger E Geisler Doug Schiavon Ricardo P Majewski Steven R Villanova Sandro Carrera Ricardo Zamora Olga Garcia Hernandez D A Shetrone Matthew Frinchaboy Peter Meza Andres Fernandez Trincado J G Munoz Ricardo R Lin Chien Cheng Lane Richard R Nitschelm Christian Pan Kaike Bizyaev Dmitry Oravetz Daniel Simmons Audrey 2016 Two groups of red giants with distinct chemical abundances in the bulge globular cluster NGC 6553 through the eyes of APOGEE Monthly Notices of the Royal Astronomical Society 465 19 31 arXiv 1610 06763 doi 10 1093 mnras stw2739 Munoz C Villanova S Geisler D Cortes C C Moni Bidin C Cohen R E Saviane I Dias B Tang B Mauro F 2019 The vertical Na O relation in the bulge globular cluster NGC 6553 Monthly Notices of the Royal Astronomical Society 492 3 3742 3752 arXiv 1912 03742 doi 10 1093 mnras stz3586 Munoz C Geisler D Villanova S Saviane I Cortes C C Dias B Cohen R E Mauro F Moni Bidin C 2018 Chemical analysis of NGC 6528 One of the most metal rich bulge globular clusters Astronomy amp Astrophysics 620 A96 arXiv 1809 04164 doi 10 1051 0004 6361 201833373 S2CID 119085692External links Edit Media related to NGC 6553 at Wikimedia Commons NGC 6553 This star cluster related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title NGC 6553 amp oldid 1141395051, wikipedia, wiki, book, books, library,

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