About the Book
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Pages: 27. Chapters: Algol variables, Beta Lyrae variables, W Ursae Majoris variables, Epsilon Ursae Majoris, Epsilon Aurigae, Alpha Coronae Borealis, SS 433, Castor, Delta Capricorni, Zeta Andromedae, Alcyone, Delta Orionis, Beta Aurigae, VV Cephei, NN Serpentis, 44 Bootis, 8 Andromedae, V415 Carinae, HW Virginis, Delta Cassiopeiae, Epsilon Carinae, KOI-81, Delta Velorum, AR Cassiopeiae, VW Cephei, DP Leonis, OY Carinae, KOI-74, Zeta Aurigae, 94 Aquarii, QS Virginis, Nu Arae, BG Geminorum, Alpha Octantis, YZ Cassiopeiae, Zeta Cygni, WW Aurigae, Zeta Tauri, Lambda Tauri, WZ Cephei, HU Aquarii, Mu Sagittarii, 29 Aquarii, Tau Arietis, Y Sextantis, Eta Orionis, QS Aquilae, Delta Equulei, Omicron Andromedae, Black Widow Pulsar, AR Aurigae, 17 Lyrae, 86 Aquarii, 31 Camelopardalis, HD 172044, Z Chamaeleontis, Upsilon Sagittarii, 9 Andromedae, Sigma Scorpii, Sigma Aquilae, HR 6902, Xi Tauri, HD 139691, 3 Centauri, LH54-425, BD+05 706, Epsilon Ursae Minoris, Tau Canis Majoris, LY Aurigae, Omicron2 Cygni, Pi Scorpii, V420 Aurigae, Mu Scorpii, DV Aquarii, R Canis Majoris, EO Aurigae, R Arae, HD 126200, V357 Carinae, WASP-9, Psi Virginis, S Antliae, 29 Canis Majoris. Excerpt: Epsilon Aurigae ( Aur, Aurigae) is a star in the constellation Auriga. It is traditionally known as Almaaz, Haldus, or Al Anz. Epsilon Aurigae is an unusual eclipsing binary system comprising an F0 supergiant and a companion which is generally accepted to be a huge dark disk orbiting an unknown object, possibly a binary system of two small B-type stars. About every 27 years, Epsilon Aurigae's brightness drops from an apparent visual magnitude of +2.92 to +3.83. This dimming lasts 640-730 days. In addition to this eclipse, the system also has a low amplitude pulsation with a non-consistent period of around 66 days. The distance to the system is still a subject of debate, ...