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Star in the constellation Auriga
36 Aurigae is a single variable star located about 1030 light years away from the Sun in the constellation Auriga. It has the variable star designation
36_Aurigae
Constellation in the northern celestial hemisphere
Aurigae. SIMBAD Kappa Aurigae. SIMBAD Pi Aurigae. SIMBAD Tau Aurigae. SIMBAD Upsilon Aurigae. SIMBAD Chi Aurigae. SIMBAD 2 Aurigae. SIMBAD Mu Aurigae
Auriga
Star in the constellation Taurus
Tauri and abbreviated Beta Tau or β Tau. The original designation of Gamma Aurigae is now rarely used. It is a chemically peculiar B7 giant star, 134 light
Beta_Tauri
Star in the constellation Andromeda
2005), "uvby FCAPT Photometry of the Magnetic Chemically Peculiar Stars 36 Aurigae, HR 2722, 13 Andromedae, and HD 220147", The Publications of the Astronomical
13_Andromedae
Star in the constellation Auriga
NO Aurigae is a pulsating variable star in the constellation Auriga. It is an unusually luminous asymptotic giant branch star about 3,500 light-years
NO_Aurigae
Brightest star in the constellation Auriga
constellation of Auriga. It has the Bayer designation α Aurigae, which is Latinised to Alpha Aurigae and abbreviated Alpha Aur or α Aur. Capella is the sixth-brightest
Capella
Star in the constellation Perseus
1 Aurigae is the original name for a star now in the constellation Perseus. It was the first entry in John Flamsteed's catalogue of stars in Auriga. When
1_Aurigae
Star in the constellation Auriga
V352 Aurigae is a variable star in the northern constellation of Auriga. It dimly visible to the naked eye with an apparent visual magnitude that ranges
V352_Aurigae
Emission and reflection nebula in the constellation Auriga
celestial equator, surrounding the bluish, irregular variable star AE Aurigae. It shines at magnitude +6.0. Its celestial coordinates are RA 05h 16.2m
IC_405
Star in the constellation Auriga
Psi4 Aurigae is a single, orange-hued star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ4 Aurigae, and
Psi4_Aurigae
Star in the constellation Auriga
Psi5 Aurigae is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ5 Aurigae, and abbreviated Psi5
Psi5_Aurigae
Solar analog star in the constellation Auriga
Lambda Aurigae is a Sun-like star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from λ Aurigae, and abbreviated
Lambda_Aurigae
Star in the constellation Auriga
Omicron Aurigae is an astrometric binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ο
Omicron_Aurigae
Possible binary star system in the constellation Auriga
2 Aurigae is a possible binary star system in the northern constellation of Auriga. This object is visible to the naked eye as a faint, orange-hued star
2_Aurigae
Star in the constellation Auriga
Upsilon Aurigae is a single star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinised from υ Aurigae, and abbreviated
Upsilon_Aurigae
Binary star in the constellation Auriga
Psi6 Aurigae is a spectroscopic binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ6
Psi6_Aurigae
Star in the constellation Auriga
Aurigae is a candidate binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from μ Aurigae,
Mu_Aurigae
Young stars of spectral types A and B
include: HD 95086 b around an A-type star HD 100546 b around a B-type star AB Aurigae b around an A-type star IRAS 12196-6300 is located just under 2300 light-years
Herbig_Ae/Be_star
Star in the constellation Auriga
Xi Aurigae is a single, white-hued star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ξ Aurigae, and
Xi_Aurigae
Type of large cool star
Arcturus is 36 light-years away. Aldebaran (α Tauri) Arcturus (α Bootis) μ Leonis Gacrux (γ Crucis) Pollux (β Geminorum) Capella Aa (α Aurigae) Schedar (α
Red_giant
Star in the constellation Gemini
cannot be observed with the naked eye. The closest star to Gliese 251 is QY Aurigae, which is located 3.5 light years away. Gliese 251 is a red dwarf with
Gliese_251
Star in the constellation Auriga
63 Aurigae is a single star located around 395 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as
63_Aurigae
T Tauri star; Chamaeleon
36: 57. Bibcode:1979A&AS...36...57B. ISSN 0365-0138. S2CID 118968842. Glass, I. S.; Pension, M. V. (1 May 1974). "An Infrared Survey of RW Aurigae Stars"
T_Chamaeleontis
Emission nebula in the constellation of Orion
which may have also created several known runaway stars, including AE Aurigae, Mu Columbae and 53 Arietis, which are believed to have been part of a
Barnard's_Loop
Eclipsing binary star of Algol type in the constellation Auriga
EO Aurigae is an eclipsing binary of Algol type in the northern constellation of Auriga. With a combined apparent magnitude of 7.71, it is too faint to
EO_Aurigae
Publications of the Astronomical Society of the Pacific. 36 (211): 124–130. Bibcode:1924PASP...36..124A. doi:10.1086/123392. JSTOR 40692425. "NameExoWorlds
List_of_proper_names_of_stars
Multiple star system in the constellation Auriga
9 Aurigae (9 Aur) is a star system in the constellation Auriga. It has an apparent magnitude of about 5, making it visible to the naked eye in many suburban
9_Aurigae
Star in the constellation Auriga
66 Aurigae (also named fyozai) is a single star located approximately 880 light years away from the Sun in the northern constellation of Auriga. It is
66_Aurigae
Diffuse nebula in the constellation Orion
the Orion Nebula cluster may have been the home of the runaway stars AE Aurigae, 53 Arietis, and Mu Columbae, which are currently moving away from the
Orion_Nebula
Binary star system in the constellation Auriga
Gliese 268 (QY Aurigae) is a binary star system in the constellation of Auriga, and is one of the one hundred closest star systems to the Earth, at a
Gliese_268
Binary star in the constellation Auriga
LY Aurigae is a multiple star system in the constellation Auriga. It is an eclipsing binary variable star, dropping in brightness by 0.7 magnitudes every
LY_Aurigae
including Antares and 119 Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements
List_of_largest_stars
Binary star system in the constellation Auriga
65 Aurigae is a binary star system located 252 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as
65_Aurigae
Star in the constellation Auriga
19 Aurigae is a single star located approximately 3,800 light years away from the Sun in the northern constellation Auriga. It is visible to the naked
19_Aurigae
Binary star system in the constellation Auriga
41 Aurigae is a binary star system located around 310–316 light years away from the Sun in the northern constellation of Auriga. It is visible to the
41_Aurigae
Small number of stars that orbit each other
star groups or a multiple system. This event is credited with ejecting AE Aurigae, Mu Columbae and 53 Arietis at above 200 km·s−1 and has been traced to
Star_system
Stellar classification distinguished by bright blue luminosity
remain unchanged since at least the 1940s, are Upsilon Orionis (B0 V), Eta Aurigae (B3 V), and Alkaid (B3 V). Besides these anchor standards, the seminal
B-type_main-sequence_star
Triple star system in the constellation Auriga
AR Aurigae (AR Aur), also known by its Flamsteed designation 17 Aurigae, is a triple star in the constellation Auriga. Based on parallax measurements made
AR_Aurigae
07var) Vega α Lyrae 0025 A0Va Northern 6 0.08 (0.03–0.16var) Capella α Aurigae 0043 K0 III, G1 III Northern 7 0.13 (0.05–0.18var) Rigel β Orionis 0860
List_of_brightest_stars
Red supergiant star in the constellation Orion
supernovae, and there is strong evidence that OB stars μ Columbae, AE Aurigae, and 53 Arietis all originated from such explosions in Ori OB1 2.2, 2.7
Betelgeuse
Brightest star in Earth's night sky
proposed Sirius Supercluster, along with other scattered stars such as Beta Aurigae, Alpha Coronae Borealis, Beta Crateris, Beta Eridani and Beta Serpentis
Sirius
Constellation in the northern celestial hemisphere
"Properties of main-sequence eclipsing binaries - Into the G stars with HS Aurigae, FL Lyrae, and EW Orionis". The Astronomical Journal. 91: 383. Bibcode:1986AJ
Lyra
Large planetary embryo
formation for a gas giant. It is located in the gas disk of the star AB Aurigae. AB Aur b is among the largest exoplanets identified, and has a distant
Protoplanet
Star in the constellation Auriga
V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11, so it is faintly visible
V394_Aurigae
Type of star larger than main-sequence but smaller than a giant
Pegasi, ζ Cassiopeiae, η Lyrae B3: ι Herculis, η Aurigae B5: τ Herculis, δ Persei, CH Crucis A2: β Aurigae, λ Ursae Majoris, β Serpentis, α Ophiuchi A3:
Subgiant
Mystery religion in the Roman Empire
iconography of Cautes and Cautopates: The data". Journal of Mithraic Studies. 1: 36–67. See also Malandra, William W. "Cautes and Cautopates". Encyclopædia Iranica
Mithraism
Zodiac constellation straddling the celestial equator
constellation of Auriga. As a result, it also bears the designation Gamma Aurigae. Zeta Tauri (the proper name is Tianguan) is an eclipsing binary star that
Taurus_(constellation)
b) 9 Aurigae C (V398 Aurigae) 87.65 ± 0.04 Auriga 05h 06m 40.62967s +51° 35′ 51.8025″ K5Ve 4.93 - 5.03 15 Pegasi 87.8 ± 0.12 F2V 5.53 9 Aurigae (V398
List of star systems within 85–90 light-years
List_of_star_systems_within_85–90_light-years
Brightest star in the constellation Lyra
FIRST: First on-sky demonstration on Keho'oea (α Lyrae) and Hokulei (α Aurigae)". Astronomy & Astrophysics. 677: A84. arXiv:2307.09746. Bibcode:2023A&A
Vega
Organization of amateur and professional astronomers
collaboration project examining the 2009-2011 eclipse of the star epsilon Aurigae. The AAVSO headquarters was originally located at the residence of its
American Association of Variable Star Observers
American_Association_of_Variable_Star_Observers
8 T7 Psi5 Aurigae 53.9 ± 0.6 Auriga 06h 46m 44.337s +43° 34′ 38.73″ G0V 5.25 HD 53705/53706/53680 53.9 ± 0.9 Puppis 07h 03m 57.315s −43° 36′ 28.93″ GV
List of star systems within 50–55 light-years
List_of_star_systems_within_50–55_light-years
A:G3III: (G8III + G0III) H:M2.5 V L:M4: 196 HD 33564 Camelopardalis 67.8 ± 0.1 5.08 F7V b 197 Lambda Aurigae Auriga 40.97 ± 0.05 4.71 G1 V or G1.5 IV-V Fe-1
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Exoplanets confirmed or discovered from direct imaging
"Images of embedded Jovian planet formation at a wide separation around AB Aurigae". Nature Astronomy. 6 (6). Springer Science and Business Media LLC: 751–759
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
Star in the constellation Auriga
HD 34626, also known as MZ Aurigae, is an unusual variable star in the northern constellation of Auriga. It has an apparent magnitude of 8.2 and is about
HD_34626
Daniel J.; Shappee, Benjamin J. (May 2016). "An extreme analogue of ε Aurigae: an M-giant eclipsed every 69 years by a large opaque disk surrounding
List_of_nearest_hypergiants
J.; Turner, N.; Pedretti, E.; Thureau, N. (2015). "Interferometry of ɛ Aurigae: Characterization of the Asymmetric Eclipsing Disk". The Astrophysical
List of stars with resolved images
List_of_stars_with_resolved_images
Cloud Galaxy 1.88 Alpha Trianguli Australis (Atria) Star 1.90 1.89 Beta Aurigae (Menkalinan) Binary star system 1.918 Alpha Pavonis (Peacock) Binary star
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Encountering with the Solar System". Astronomy Letters. 36 (3): 220–226. arXiv:1003.2160. Bibcode:2010AstL...36..220B. doi:10.1134/S1063773710030060. S2CID 118374161
List_of_nearest_stars
Study of the movement of stars
process. An example of a related set of runaway stars is the case of AE Aurigae, 53 Arietis and Mu Columbae, all of which are moving away from each other
Stellar_kinematics
HR 483 A 41.2 ± 0.4 Andromeda 01h 41m 47.1431s +42° 36′ 48.444″ G1.5V 4.95/12.5 B MV Lambda Aurigae (Al Hurr)$ 41.2 ± 0.5 Auriga 05h 19m 08.475s +40° 05′
List of star systems within 40–45 light-years
List_of_star_systems_within_40–45_light-years
members include Alpha Coronae Borealis (α CrB or Alphecca or Gemma), Beta Aurigae (β Aur), Delta Aquarii (δ Aqr), Gamma Leporis (γ Lep) and Beta Serpentis
Ursa_Major_moving_group
Taurus; also known as 112 Tauri In Auriga In Auriga, also known as 30 Aurigae In Lynx In Ursa Major In Gemini In Coma Berenices In Columba In Pisces;
Table of stars with Flamsteed designations
Table_of_stars_with_Flamsteed_designations
Triple star system in the constellation Cygnus
Eaton, Joel A.; et al. (2008). "Orbits and Pulsations of the Classical ζ Aurigae Binaries". The Astrophysical Journal. 679 (2): 1490–1498. arXiv:0802.2238
31_Cygni
3 2 O9.5V 4.07 Meissa A (Lambda Orionis) 1260±200 1 O8 III((f)) 3.7 AE Aurigae 1,320 ± 40 1 O9.5V 5.96 Xi Persei (Menkib) 1,340±65 1 O7.5III(n)((f)) 4
List_of_O-type_stars
List of largest planets by size
"Images of embedded Jovian planet formation at a wide separation around AB Aurigae". Nature Astronomy. 6 (6): 751–759. arXiv:2204.00633. Bibcode:2022NatAs
List_of_largest_exoplanets
772 9 , 160 ) 4 ⋅ 10 1.36 = 1.9 R ⊙ . {\displaystyle {\sqrt {{\biggl (}{\frac {5,772}{9,160}}{\biggr )}^{4}\cdot 10^{1.36}}}=1.9\ R_{\odot }.} Applying
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
813s +19° 17′ 37.88″ A0Vnp λ Boo or A0IV-V(n)kB8 3.86 B A2IVpSiSrCr Theta Aurigae (Mahasim) A 166 ± 1 Auriga 05h 59m 43.27012s +37° 12′ 45.3047″ A0pSi 2
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Binary star in the constellation Cepheus
the exact onset is difficult to measure because it is gradual. Only ε Aurigae (period = 27.08 years), and AS Leonis Minoris (period = 69.1 years) have
VV_Cephei
Type of variable star
Camelopardalis 5m.15 5m.27 0.12 M0 II Lc Pi Aurigae Auriga 4m.24 4m.34 0.10 M3.5 II Lc NO Aurigae Auriga 6m.06 6m.44 0.58 M2 Iab Lc Omicron1
Slow_irregular_variable
Aquarius B5 III 5.43 V357 Carinae 450 ± 20 Carina B2IV-V +3.41 - 3.44 Iota Aurigae (Hassaleh) 450 ± 20 Auriga K3 II–III 2.69 28 Monocerotis 450 ± 20 Monoceros
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
previously been recorded of having a parallax of 127 mas. Capella (Alpha Aurigae) Star 1849–1891 72 ly (46 mas) Polaris (Alpha Ursae Minoris) Star 1847–1849
List of the most distant astronomical objects
List_of_the_most_distant_astronomical_objects
Star whose atmosphere contains more carbon than oxygen
Review of Astronomy and Astrophysics. 36 (1): 369–433. Bibcode:1998ARA&A..36..369W. doi:10.1146/annurev.astro.36.1.369. Zinner, E. (1 January 2014). "1
Carbon_star
Quasar in the constellation Auriga
constellation Auriga not far in the sky from the 5th magnitude star Omicron Aurigae. The "distance" of a far away galaxy depends on the distance measurement
3C_147
Unique identifier given to variable stars
to 45,678 variable stars. Among the newly designated objects were V0654 Aurigae, V1367 Centauri, and BU Coronae Borealis. Most of this system was invented
Variable-star_designation
American astronomer
star clusters such as Omega Centauri, Alpha Centauri, M5, and Epsilon Aurigae. In 1903, she and Williamina Fleming investigated the possibility of a
Evelyn_Leland
Star in the constellation Auriga
47 Aurigae is a star located around 680 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim
47_Aurigae
Benjamin J.; Kochanek, Christopher S. (April 2016). "AN EXTREME ANALOGUE OF ϵ AURIGAE: AN M-GIANT ECLIPSED EVERY 69 YEARS BY A LARGE OPAQUE DISK SURROUNDING
List_of_smallest_known_stars
Rigel β Orionis foot (left foot of Orion) 282 S 08° 0.12 12 Capella α Aurigae little she-goat 281 N 46° 0.71 13 Bellatrix γ Orionis female warrior 279
List_of_stars_for_navigation
Star that is particularly similar to the Sun
1051/0004-6361:200809698. S2CID 18173201. See VizieR catalogue J/A+A/487/373. V538 Aurigae at SIMBAD - Ids - Bibliography - Image. HD 14412 at SIMBAD - Ids - Bibliography
Solar_analog
Pyxidis) 39.7 ± 0.3 Pyxis 08h 32m 51.49609s -30° 31′ 03.0717″ G9V 6.38 V538 Aurigae 39.9 ± 0.4 Auriga 05h 41m 20.33573s +53° 28′ 51.8106″ K1V 6.25 System Star
List of star systems within 35–40 light-years
List_of_star_systems_within_35–40_light-years
Miki (2004-04-01). "Spiral Structure in the Circumstellar Disk around AB Aurigae". The Astrophysical Journal. 605 (1): L53–L56. Bibcode:2004ApJ...605L.
List of resolved circumstellar disks
List_of_resolved_circumstellar_disks
Herbig Ae star in the constellation Sagittarius
Ultraviolet Explorer, showing that it is similar to the Herbig Ae star AB Aurigae. Observations with Hubble STIS showed Herbig-Haro nebulosity that is often
HD_163296
Non-periodic comet
Wilson noted a light source that looked like a searchlight next to theta Aurigae. He examined it with binoculars as it rose above the horizon and found
C/1961_O1_(Wilson–Hubbard)
Month of 1974
Richard Catura detected x-ray luminosity from the star Capella (Alpha Aurigae), almost 43 light years from Earth, that was more than 10,000 times as
April_1974
astronomer Antonia Maury discovered the second spectroscopic binary, Beta Aurigae, and calculated its orbital period. 1889: American geologist Mary Emilie
Timeline_of_women_in_science
−12° 37′ 55.8″ 41.0 Gliese 67 A G1.5V 4.95 4.30 01h 41m 47.1s +42° 36′ 48.1″ 41.2 λ Aurigae G0V 4.69 4.18 05h 19m 08.38s +40° 05′ 56.6″ 41.2 HD 14412 (22 G
List_of_nearest_bright_stars
massive star within 2,500 light-years followed by 68 Cygni with a mass of 36+14 −10 M☉ and other nearby massive stars. The minimum mass is between 8 to
List_of_nearest_massive_stars
Star in the constellation Taurus
Hoffmeister in 1949. Hoffmeister classified it as a member of the RW Aurigae-like variables with a brightness that ranged from an apparent visual magnitude
CQ_Tauri
Type of variable star
Cygni 7.1 14.7 264 654+36 −33 [57] S Orionis 7.2 13.1 434 538+120 −83 [58] T Draconis 7.2 13.5 422 783+48 −43 [59] UV Aurigae 7.3 10.9 394 1107+83 −72
Mira_variable
95 Part of Coma Star Cluster. K2-155 267 K7 Has 3 exoplanets. 14 Aurigae (KW Aurigae) A 269 ± 4 Auriga A9IV + ? 5.01 B F5V C M3V: D WDA K2-384 270 M0V
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
Antonio; Pavlovski, Kresimir; Dotter, Aaron (2015-05-27), "Capella (alpha Aurigae) revisited: New binary orbit, physical properties, and evolutionary state"
List_of_nearest_giant_stars
Roman-era mosaic
of Barb breed horses, while five depict sparsores (water-sprinklers) or aurigae (charioteers). The horses are positioned facing left or right, almost all
Mosaic of the Horses of Carthage
Mosaic_of_the_Horses_of_Carthage
Astronomy catalogue
vdB 26 vdB 27 vdB 28 vdB 29 vdB 30 vdB 31 vdB 32 vdB 33 vdB 34 vdB 35 vdB 36 vdB 37 vdB 38 vdB 39 vdB 40 vdB 41 vdB 42 vdB 43 vdB 44 vdB 45 vdB 46 vdB
Van_den_Bergh_Catalog
9 V398 32537 23783 05h 06m 40.66s +51° 35′ 53.3″ 4.98 2.89 85 F0V V398 Aurigae, Gamma Doradus variable, Vmax = 4.93m, Vmin = 5.03m, P = 1.25804 d ψ7 Aur
List_of_stars_in_Auriga
Multiple star system in the constellation of Chamaeleon
and its spectrum closely resembles other Herbig Ae/Be stars such as AB Aurigae and HR 5999. No characteristic molecular cloud was detected nearby, although
HD_104237
listing is only for additional stars Other designation of this star is Psi10 Aurigae (ψ10 Aur) the star is actually located in the constellation Lynx near the
Lynx_in_Chinese_astronomy
Canopus (fourth time) +480,000 +990,000 +480,000 −0.40 346 310 −0.72 Beta Aurigae (Menkalinan) +990,000 +1,150,000 +1,190,000 −0.40 28.5 82.1 1.9 Delta Scuti
Historical_brightest_stars
Draconis 1,850 C6,2e V346 Puppis 1,875 C Leo A 22 1,900 C 2,600,000 S Aurigae 1,940 C-N5+ V1426 Cygni 1,975 C7,2e Sextans A 20 2,000 C 4,310,000 Leo
List_of_coolest_stars
e037. arXiv:2206.04204. Bibcode:2022PASA...39...37O. doi:10.1017/pasa.2022.36. S2CID 249538461. "Appetite-suppressing molecule helps obese mice lose weight"
2022_in_science
Star system in the constellation Perseus
shown to undergo such large adjustments in eclipse amplitude after IU Aurigae. The changes suggested a wobble in the orbital plane caused by an orbiting
RW_Persei
travel, tourism, insurance
36 AURIGAE
36 AURIGAE
Surname or Lastname
English
English : from the Middle English vernacular form of the personal name Barnabas, which was borne by the companion of St Paul (Acts 4:36). This is of Aramaic origin, from Barnabia ‘son of Nabia’, a personal name perhaps meaning ‘confession’.English : habitational name from Barnaby in North Yorkshire, named with the Old English personal name Beornwald (composed of the elements beorn ‘young warrior’ + wald ‘rule’) + Old Norse býr ‘settlement’.
Boy/Male
Muslim
One of the prophet muhammads names, Victory, The two opening letters of surah 36 in the Quran
Female
English
(Aramaic טַבְיְתָ×, Greek: Ταβιθά, Hebrew: צְבִיָּה): Greek name of Aramaic origin, TABITHA means "female gazelle." In the New Testament bible, this is the name of a woman restored to life by Peter. The name was translated as Dorkas in Acts 9:36.
Boy/Male
Muslim
One of the prophet muhammads names, Victory, The two opening letters of surah 36 in the Quran
36 AURIGAE
36 AURIGAE
36 AURIGAE
36 AURIGAE
36 AURIGAE
36 AURIGAE
36 AURIGAE
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