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The radiant point for this shower passes several degrees to the south of the star. [12] The variable radial velocity of this system was not recognized until 1999, more than a century following the first measurement in 1897. Delta Aurigae is a single-lined spectroscopic binary: periodic Doppler shifts in the star's spectrum indicate orbital motion.
41 Aurigae is a binary star [10] system located around 310–316 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim, white-hued star with a combined apparent visual magnitude of 5.83. [10] This system is moving further from the Earth with a heliocentric radial velocity of 31 km/s. [11]
65 Aurigae is a binary star [7] system located 252 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a faint, orange hued star with an apparent visual magnitude of 5.12. [2] The primary, designated component A, is an aging giant star with a stellar classification of K0 III. [3]
16 Aurigae is a triple star [12] system located 232 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.547, [ 13 ] and is located about 2/3 of the way from Capella toward Beta Tauri .
43 Aurigae is a star located 382 light years away from the Sun in the northern constellation of Auriga. It is just bright enough to be barely visible to the naked eye with an apparent visual magnitude of 6.33. [2] The star is moving closer to the Earth with a heliocentric radial velocity of −3.4 km/s. [2]
45 Aurigae or PLX 1468.2 is a binary star [5] system in the northern constellation of Auriga. It has an apparent visual magnitude of 5.34, [2] making it visible to the naked eye under suitable viewing conditions. An annual parallax shift of 16.89 mas as seen from Earth's orbit indicates the system is located about 193 light years from the Sun.
Psi 6 Aurigae, Latinized from ψ 6 Aurigae, is a spectroscopic binary [5] star in the northern constellation of Auriga. It is a dim, naked eye star with an apparent visual magnitude of +5.22. [ 2 ] Based upon a measured annual parallax shift of 9.05 ± 0.38 mas , [ 1 ] it is approximately 360 light-years (110 parsecs ) distant from the Earth.
9 Aurigae (9 Aur) is a star system in Auriga (constellation).It has an apparent magnitude of about 5, making it visible to the naked eye in many suburban skies. [15] Parallax estimates made by the Hipparcos spacecraft put it at about 86 light-years (26 parsecs) from the solar system, [1] although individual Gaia Data Release 3 parallaxes place all three components at 88 light years.
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