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Dense star cluster of massive young stars in the constellation of Sagittarius
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
Quintuplet_Cluster
Topics referred to by the same term
of equal duration The Quintuplet Cluster, a star cluster near the Galactic Center Quintuplets, an American sitcom "Quintuplets 2000", an episode of the
Quintuplet_(disambiguation)
Stars sorted by absolute magnitude
Hamann, W. -R.; Oskinova, L. M.; Todt, H.; Butler, K. (2010). "The Quintuplet cluster". Astronomy & Astrophysics. 524: A82. arXiv:1011.5796. Bibcode:2010A&A
List_of_most_luminous_stars
Hypergiant star in Sagittarius
stars 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
Pistol_Star
infrared cluster is a type of star cluster only visible in infrared light. Prominent examples include the Quintuplet Cluster, Arches Cluster and central
Infrared_cluster
Luminous blue variable star in the constellation Sagittarius
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
V4998_Sagittarii
Densest star cluster known
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
Arches_Cluster
List of globular clusters Lists of clusters Figer, Donald F.; McLean, Ian S.; Morris, Mark (1999). "Massive Stars in the Quintuplet Cluster". The Astrophysical
List_of_infrared_clusters
Nebula around the Pistol Star
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
Pistol_Nebula
Luminous blue variable star in the constellation Sagittarius
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
V4650_Sagittarii
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
List_of_most_massive_stars
American astronomer
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
Donald_Figer
include Antares, Spica, Gamma Velorum, Mu Cephei, and members of the Quintuplet Cluster. Type Ia supernova progenitors are white dwarf stars that are close
List_of_supernova_candidates
Multiple star system in the constellation Carina
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
HD_97950
Star in the constellation Sagittarius
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
WR_102ea
Wolf-Rayet star
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
WR_102c
This is a list of open clusters located in the Milky Way. An open cluster is an association of up to a few thousand stars that all formed from the same
List_of_open_clusters
the Quintuplet Cluster LBV G0.120-0.048 (V4998 Sgr) 26,000 WN5b near the Quintuplet Cluster FMM 362 (V4650 Sgr) 26,000 LBV near the Quintuplet Cluster AFGL
List of luminous blue variable stars
List_of_luminous_blue_variable_stars
Type of star that is luminous, blue, and variable in brightness
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
Luminous_blue_variable
S2CID 11060463. Liermann, A.; Hamann, W.-R.; Oskinova, L. M. (2009). "The Quintuplet cluster". Astronomy and Astrophysics. 494 (3): 1137. arXiv:0809.5199. Bibcode:2009A&A
List_of_stars_in_Sagittarius
Millisecond pulsar candidate in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Breakthrough_Listen_Pulsar
Binary star system in which two massive stars emit powerful stellar winds
nebula of spiraling dust. Such pinwheels have been observed in the Quintuplet Cluster. The archetype of such a colliding-wind binary system is WR 140 (HD
Colliding-wind_binary
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Beta2_Sagittarii
Index of articles associated with the same name
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Beta_Sagittarii
Triple star system in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Nu1_Sagittarii
Way. WR 102ka (Peony Star) 26,000 Ofpe/WN9 WR 102c WN6 11.6 Part of Quintuplet cluster. WR 102ea WN9h 8.8 WR 102da WC9?d WR 102dc WC9d + OB WR 102ha WC8/9d
List_of_Wolf–Rayet_stars
Astrometric binary star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Iota_Sagittarii
Index of articles associated with the same name
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Kappa_Sagittarii
Index of articles associated with the same name
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Chi_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Chi3_Sagittarii
Index of articles associated with the same name
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Theta_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Xi2_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
HD_167665
Index of articles associated with the same name
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Nu_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Xi1_Sagittarii
Star in the constellation Sagittarius
velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations", Astronomische Nachrichten, 328 (9): 889–896, arXiv:0705
Chi1_Sagittarii
Binary star system in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Theta1_Sagittarii
Binary star system in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Beta1_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
HD_165185
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Nu2_Sagittarii
B-type main sequence star in the constellation Sagittarius
velocities of ̃55000 stars and mean radial velocities of 516 Galactic open clusters and associations", Astronomische Nachrichten, 328 (9): 889, arXiv:0705
HD_182681
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Kappa2_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Xi_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Theta2_Sagittarii
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Rho2_Sagittarii
Binary star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Kappa1_Sagittarii
Herbig Ae star in the constellation Sagittarius
(2024-06-01). "Improving the open cluster census. III. Using cluster masses, radii, and dynamics to create a cleaned open cluster catalogue". Astronomy and Astrophysics
HD_163296
Star in the constellation Sagittarius
Messier 28 Messier 54 Messier 55 Messier 69 Messier 70 Messier 75 Quintuplet Cluster Small Sagittarius Star Cloud Terzan 5 Terzan 7 Terzan 8 VVV CL001
Rho1_Sagittarii
Symbols (Unicode block) Musical Symbols (disambiguation) Shape note Tone cluster "Music Notation and Engraving – Braces and Bracket, Colorado College Music
List_of_musical_symbols
1966 choral piece by György Ligeti
cloudiness it is possible to discern a new interval combination taking shape." Cluster chords, where every note within a given interval is sung simultaneously
Lux_Aeterna_(Ligeti)
integral spin of either 2 (d-boson) or 0 (s-boson). They correspond to a quintuplet and singlet, i.e. 6 states. It is sometimes known as the Interacting boson
Interacting_boson_model
Fictional comic book program
(May 2004), Grant Morrison's last issue of New X-Men, the telepathic quintuplets called the Stepford Cuckoos were identified as Weapon XIV. The Stepford
Weapon_Plus
COVID-19". Anime News Network. Retrieved April 26, 2020. "The Quintessential Quintuplets Anime Season 2 Delayed to January 2021 Due to COVID-19". Anime News Network
Impact of the COVID-19 pandemic on television
Impact_of_the_COVID-19_pandemic_on_television
and leakage power consumed by the circuit. An FSM can be defined as a quintuplet that consists of a set of primary inputs, a set of primary outputs, a
Low-power_FSM_synthesis
Musical style of composer Béla Bartók
the Sonata for two pianos and percussion. This motive is scored as a quintuplet of sixteenths in 4 4 time on the third beat, plus a sixteenth note on
Night_music_(Bartók)
1916 composition by Henry Cowell
piece is also noted for its extended use of tuplets, featuring triplets, quintuplets, and sextuplets in the melody line. While still a teenager and studying
Dynamic_Motion
Five pieces for piano (1926) by Béla Bartók
spanning an augmented octave The left hand plays an ostinato arpeggiated quintuplet chord of F, G♯, B, C♯, E, of which the E is on the beat (6 8 measure)
Out_of_Doors_(Bartók)
English, as in American English (paralleling, unparalleled), to avoid the cluster -llell-. Words with two vowels before a final l are also spelled with -ll-
American and British English spelling differences
American_and_British_English_spelling_differences
August 1954). "Emilie Dionne Laid To Rest Amid Bitter Sobs Of Surviving Quintuplets". The Newport Daily News. Warner, Jack. "The Village Eccentric on Trial"
List_of_people_with_epilepsy
Oto-Manguean language branch of Mexico
phonological innovations, Rensch (1989) groups the Chinantecan languages into 5 clusters, which largely agree with previous ethnographic classifications of the
Chinantecan_languages
Piano composition by Samuel Barber
rhythm in the right hand. At the same time, the eighth-note followed by a quintuplet pattern continues. This variation is similar to variation I in this manner
Excursions_(Barber)
Series of compositions by Karlheinz Stockhausen
equal parts. Of these five divisions, the dominating one is the rising quintuplet in the Lucifer layer of the most-background layer, each note of which
Klavierstücke_(Stockhausen)
suspended from holding his post with immediate effect. 28 August Girl quintuplets are born at the De Soysa Hospital. The Ministry of Education announces
2020_in_Sri_Lanka
Bantu language of DR Congo
difference between different words and forms, as seen in the minimal quintuplet here: When a contour tone is followed by another tone that begins with
Nzadi_language
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