Tarazed, Reda, gam Aql, γ Aql, 50 Aql, BD+10 4043, FK5 741, HD 186791, HIP 97278, HR 7525, SAO 105223[9]
Database references
SIMBAD
data
Gamma Aquilae, Latinized from γ Aquilae, and formally known as Tarazed/ˈtærəzɛd/,[10] is a star in the constellation of Aquila. It has an apparent visual magnitude of 2.712,[2] making it readily visible to the naked eye at night. Parallax measurements place it at a distance of 395 light-years (121 parsecs) from the Sun.[1]
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^"IAU Catalog of Star Names". Retrieved 28 July 2016.
GammaAquilae, Latinized from γ Aquilae, and formally known as Tarazed /ˈtærəzɛd/, is a star in the constellation of Aquila. It has an apparent visual...
tarāzū (or possibly šāhīn tara zed; see GammaAquilae), the Persian name for the asterism α, β and γ Aquilae.[citation needed] In 2016, the IAU organized...
Binary star system 2.72 GammaAquilae Star 2.73 Iota Centauri Star 2.75 Delta Ophiuchi Star Suspected variable star 2.74 Gamma Virginis Binary star system...
ridgepole"; it might also mean "heavenly drumsticks", with Altair, Beta Aquilae and GammaAquilae being the drum. This distance to this star can be determined through...
δ Aquilae, μ Aquilae, σ Aquilae, ν Aquilae, ι Aquilae, 42 Aquilae, HD 184701, κ Aquilae and 56 Aquilae. Consequently, the Chinese name for δ Aquilae itself...
were studied by Mordehai Milgrom in 1979. SS 433, also known as V1343 Aquilae, located in the galactic plane (l= 39.7° and b= -2.2°), at a distance of...
Sagittae, δ Sagittae, ζ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently, the Chinese name for γ Sagittae itself is 左旗五 (Zuǒ Qí wǔ...
V923 Aquilae is a variable binary star system in the equatorial constellation of Aquila. It has the designation HD 183656 from the Henry Draper Catalogue;...
19 Aquilae is a single star located 142 light-years (44 parsecs) away from the Sun in the equatorial constellation of Aquila. 19 Aquilae is the Flamsteed...
dwarf orbiting around it. Zeta Delphini B has a mass of 50±15 MJ. Rho Aquilae at magnitude 4.94 is at about 150 light-years away. Due to its proper motion...
Archived from the original on 2020-10-08 – via IanRidpath.com. "Gacrux/Gamma Crucis 2?". Sol Station. Sol Company. Archived from the original on 2011-11-03...
within the constellation for which they are named. The proper motion of Rho Aquilae, for example, carried it across the boundary into Delphinus in 1992. A...
(2007). "Multiperiodic pulsations in the Be stars NW Serpentis and V1446 Aquilae". Astronomy and Astrophysics. 472 (2): 565–570. Bibcode:2007A&A...472....
at Pretoria Boys High School from 1917 to 1921. The appearance of Nova Aquilae (a bright nova occurring in the constellation Aquila) in 1918 and a letter...
only possibility for producing the cosmogenic isotopes. A long or short gamma-ray burst has been initially proposed as a possible cause of the AD 774/5...
"Hopkins Ultraviolet Telescope Observations of Nova Circini 1995 and Nova Aquilae 1995". Astrophysical Journal Letters. 454: L43–46. Bibcode:1995ApJ...454L...
solar. In 2010 scientists using NASA's Fermi Gamma-ray Space Telescope discovered that a nova also can emit gamma rays (>100 MeV). Potentially, a white dwarf...
"Kuwano's Object" and "Kuwano's Star" have also been used to refer to V1407 Aquilae and V4021 Sagittarii, respectively. These are all named after Yoshiyuki...
On September 10, 1784, Edward Pigott detected the variability of Eta Aquilae, the first known representative of the class of Cepheid variables. However...
Description 天市左垣六 Tiān Shì Zuǒ Yuán liù the Sixth Star of Left Wall Zeta Aquilae Okab Aquila 吳越 Wú Yuè The state of Wu and Yue Left Wall (天市左垣, Tiānshìzuǒyuán)...
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