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Quintuplet cluster information


Quintuplet Cluster
Infrared image of the Quintuplet Cluster
Credit: ESA/Hubble & NASA
Observation data (J2000. epoch)
Right ascension17h 46m 13.9s[1]
Declination−28° 49′ 48″[1]
Distance26 kly (8 kpc[2])
Apparent dimensions (V)50" (2 pc)[3]
Physical characteristics
Mass10,000[3] M
Estimated age4.8 million years[4]
Dense cluster of massive young stars near the Galactic Center. Optically obscured.
Other designationsIRAS 17430-2848, G000.16-00.06
Associations
ConstellationSagittarius
See also: Open cluster, List of open clusters

The Quintuplet cluster is a dense cluster of massive young stars about 100 light years from the Galactic Center (GC). Its name comes from the fact it has five prominent infrared sources residing in it. Along with the Arches Cluster it is one of two in the immediate GC region. Due to heavy extinction by dust in the vicinity, it is invisible to optical observation and must be studied in the X-ray, radio, and infrared bands.

The Quintuplet is less compact than the nearby Arches Cluster, with fewer of the most massive and luminous stars, but it does have the distinction of hosting two of the extremely rare luminous blue variables, the Pistol Star and the less well-known qF 362 (aka V4650 Sgr), and a third just a few parsecs away.[2] It also contains a number of red supergiants, all suggesting a slightly more evolved cluster around 4 million years old.[5]

  1. ^ a b Beichman, C. A.; Neugebauer, G.; Habing, H. J.; Clegg, P. E.; Chester, Thomas J. (1988). "Infrared astronomical satellite (IRAS) catalogs and atlases. Volume 1: Explanatory supplement". Infrared Astronomical Satellite (IRAS) Catalogs and Atlases. Volume 1: Explanatory Supplement. 1. Bibcode:1988iras....1.....B.
  2. ^ a b Cite error: The named reference mauerhan was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference figer was invoked but never defined (see the help page).
  4. ^ Schneider, F. R. N.; Izzard, R. G.; De Mink, S. E.; Langer, N.; Stolte, A.; De Koter, A.; Gvaramadze, V. V.; Hußmann, B.; Liermann, A.; Sana, H. (2014). "Ages of Young Star Clusters, Massive Blue Stragglers, and the Upper Mass Limit of Stars: Analyzing Age-dependent Stellar Mass Functions". The Astrophysical Journal. 780 (2): 117. arXiv:1312.0607. Bibcode:2014ApJ...780..117S. doi:10.1088/0004-637X/780/2/117. S2CID 28410959.
  5. ^ Cite error: The named reference hr was invoked but never defined (see the help page).

and 28 Related for: Quintuplet cluster information

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Quintuplet cluster

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The Quintuplet cluster is a dense cluster of massive young stars about 100 light years from the Galactic Center (GC). Its name comes from the fact it...

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Pistol Star

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known in the Milky Way. It is one of many massive young stars in the Quintuplet cluster in the Galactic Center region. The star owes its name to the shape...

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List of most luminous stars

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"Discovery of a Luminous Blue Variable with an Ejection Nebula Near the Quintuplet Cluster". The Astrophysical Journal. 713 (1): L33–L36. arXiv:1002.3379. Bibcode:2010ApJ...

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Pistol Nebula

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Star. Both are located 25,000 light years away from Earth in the Quintuplet cluster, near the center of the Milky Way galaxy. The nebula contains approximately...

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V4998 Sagittarii

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is positioned about 7 pc (23 ly) away from a starburst cluster known as the Quintuplet cluster. It has an ejection nebula measuring over 0.8 pc in diameter...

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V4650 Sagittarii

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away, the star is positioned on the edge of a starburst cluster known as the Quintuplet cluster. V4650 Sgr was first catalogued in 1996 as star 362 in...

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List of most massive stars

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Todt, Helge (January 2011). "High-mass stars in the Galactic center Quintuplet cluster". Société Royale des Sciences de Liège, Bulletin. 80: 160–164. Bibcode:2011BSRSL...

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WR 102ea

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Sagittarius constellation. It is the third most luminous star in the Quintuplet cluster after WR 102hb. With a luminosity of 2,500,000 times solar, it is...

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List of supernova candidates

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include Antares, Spica, Gamma Velorum, Mu Cephei, and members of the Quintuplet Cluster. Type Ia supernova progenitors are white dwarf stars that are close...

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Luminous blue variable

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Sagittarii (FMM 362 or qF362, in the Quintuplet cluster) V4998 Sagittarii (LBV3, G0.120 0.048, very close to the Quintuplet cluster) Pistol star, Peony star and...

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Arches Cluster

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The star cluster is estimated to be around two and a half million years old. Although larger and denser than the nearby Quintuplet Cluster, it appears...

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WR 102c

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Sagittarius towards the galactic centre. It is only a few parsecs from the Quintuplet Cluster, within the Sickle Nebula. According to recent estimations, WR 102c...

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List of largest stars

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Rolf P. (February 2009). "Metallicity in the Galactic Center: The Quintuplet Cluster". The Astrophysical Journal. 691 (2): 1816–1827. arXiv:0809.3185....

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Chi Sagittarii

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21 Messier 22 Messier 23 Messier 25 Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet cluster Small Sagittarius Star Cloud...

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Nu1 Sagittarii

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21 Messier 22 Messier 23 Messier 25 Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet cluster Small Sagittarius Star Cloud...

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Donald Figer

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census of massive stars in both the Quintuplet Cluster and the Arches Cluster, finding that massive star clusters form in the present-day Galaxy, as opposed...

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Nu Sagittarii

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21 Messier 22 Messier 23 Messier 25 Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet cluster Small Sagittarius Star Cloud...

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Xi2 Sagittarii

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Kappa Sagittarii

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Beta Sagittarii

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Xi Sagittarii

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Beta2 Sagittarii

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HD 97950

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clusters in the galaxy. The Arches Cluster is around 2.5 million years old, the Quintuplet cluster nearly double that, and the various open clusters containing...

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Iota Sagittarii

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21 Messier 22 Messier 23 Messier 25 Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet cluster Small Sagittarius Star Cloud...

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Xi1 Sagittarii

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Nu2 Sagittarii

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Rho2 Sagittarii

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Theta2 Sagittarii

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