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Binary star in the constellation Auriga
WW Aurigae is an eclipsing binary star system in the northern constellation of Auriga. It has a combined maximum apparent visual magnitude of 5.86, which
WW_Aurigae
Type of chemically peculiar star
Bibcode:2013MNRAS.429..119P, doi:10.1093/mnras/sts318, S2CID 119231581. WW Aurigae is a binary star both of whose components are Am stars. Neiner, C; Wade
Am_star
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
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
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
American astronomer (1899–1951)
February 14, 1932" (Astronomical Journal 1932), and "The eclipsing binary WW Aurigae" (Lick Observatory Bulletin 1942). Lois Tripp Slocum died in 1951, aged
Lois_Tripp_Slocum
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
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
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
Small number of stars that orbit each other
Dordrecht. p. 68. ISBN 90-277-0885-1. Blaauw, A.; Morgan, W.W. (1954). "The Space Motions of AE Aurigae and mu Columbae with Respect to the Orion Nebula". Astrophysical
Star_system
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
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
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
Study of the movement of stars
2008-02-16. Retrieved 2008-02-25. Blaauw A.; Morgan W.W. (1954). "The Space Motions of AE Aurigae and mu Columbae with Respect to the Orion Nebula". The
Stellar_kinematics
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
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WW AURIGAE
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