known, including the yellow hypergiants Rho Cassiopeiae and V509 Cassiopeiae and white hypergiant 6 Cassiopeiae. In 1572, Tycho Brahe's supernova flared...

Gamma Cassiopeiae, Latinized from γ Cassiopeiae, is a bright star at the center of the distinctive "W" asterism in the northern circumpolar constellation...

Eta Cassiopeiae (η Cassiopeiae, abbreviated Eta Cas, η Cas) is a binary star system in the northern constellation of Cassiopeia. Its binary nature was...

although it is possible that it was recorded as a sixth magnitude star 3 Cassiopeiae by John Flamsteed. Possible explanations lean toward the idea that the...

10 Cassiopeiae (10 Cas) is a blue-white giant star in the constellation Cassiopeia, about 960 light years away. 10 Cassiopeiae is a B9 giant star. It...

64 K1III+A5eIII β Lyr variable, Vmax = 8.64m, Vmin = 9.49m, P = 32.31 d Y Cas Y 225082 00h 03m 21.47s +55° 40′ 51.8″ 8.70 M7.5e Mira variable, Vmax = 8...

SN 1572 (Tycho's Supernova, Tycho's Nova), or B Cassiopeiae (B Cas), was a supernova of Type Ia in the constellation Cassiopeia, one of eight supernovae...

Zeta Cassiopeiae, Latinized from ζ Cassiopeiae, and officially named Fulu /ˈfuːluː/, is a variable star in the constellation of Cassiopeia. It has a blue-white...

variable star CZ Cassiopeiae and the evolution of the orbit of Comet Halley. Zhang discovered three comets and is credited under the name Y. C. Chang by the...

44.9 MJ, making it a brown dwarf. Kapteyn's Star Groombridge 1830 Mu Cassiopeiae 2MASS J05325346+8246465, a possible halo brown dwarf and the first substellar...

YZ-834B, a remote-controlled toy car YZ Canis Minoris, a red dwarf star YZ Cassiopeiae, a naked-eye-visible triple star system YZ Ceti, a nearby red dwarf in...

PZ Cassiopeiae is a red supergiant star located in the constellation of Cassiopeia, and a semi-regular variable star. PZ Cassiopeiae is a luminous red...

mass-losing hot stars, but was not applied to cooler stars. In 1991, Rho Cassiopeiae was the first to be described as a yellow hypergiant, likely becoming...

ul-Khaḍib the Palm (reaching from the Pleiades) الكـــف الخضيب Beta Cassiopeiae Celbalrai Kalb ur-Rāʿī the Shepherd's Dog كلب الراعي Beta Ophiuchi Chort...

cluster GCAS – (celestial object) Gamma CASsiopeiae, a class of eruptive variable stars named after Gamma Cassiopeiae, the archetype for the class GCMS –...

supergiants Betelgeuse, Antares, and VV Cephei A; the yellow hypergiant Rho Cassiopeiae; the luminous blue variable Eta Carinae that has already produced a supernova...

Gliese 22, also catalogued V547 Cassiopeiae or ADS 440, is a hierarchical star system approximately 33 light-years away in the constellation of Cassiopeia...

('river's end'). /ˈeɪkərnɑːr/ Cassiopeia η Cassiopeiae A Achird Apparently first applied to η Cassiopeiae in the Skalnate Pleso Atlas of the Heavens published...

2024). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". arXiv:2408.02756v2 [astro-ph...

absorption lines) it is also dubbed the Spectral Gem of Southern Skies. Gamma Cassiopeiae, informally named Navi for astronaut Virgil Ivan "Gus" Grissom Iota Ursae...

With the placement of the Sun east of the magnitude 3.4 star Epsilon Cassiopeiae, nearly in front of the Heart Nebula, the "W" line of stars of Cassiopeia...

the system can be considered a sextuple. Jabbah AR Cassiopeiae V871 Centauri Gamma Cassiopeiae QZ Carinae Exoplanet Solar System The term optical multiple...

temperature into the LBV range) V509 Cassiopeiae (= HR 8752, an unusual yellow hypergiant evolving bluewards) Rho Cassiopeiae (unstable yellow hypergiant suffering...

Kovtyukh, V.; Beletsky, Y. (2013). Anchors for the cosmic distance scale: the Cepheids U Sagittarii, CF Cassiopeiae, and CEab Cassiopeiae, A&A, 260 Quinn, Samuel...

Cambridge Catalogue of Radio Sources. It is located 2° northeast of ε Cassiopeiae and is estimated to be 10,000 light-years away. Its rotation period is...

objects have also been assigned letters: D for white dwarfs and L, T and Y for Brown dwarfs. In the MK system, a luminosity class is added to the spectral...

one of which is a suspected cluster member. The eclipsing binary OX Cassiopeiae was once thought to be a member, but is now known to be a background...

Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs". The Astrophysical Journal Supplement Series. 253 (1): 7. arXiv:2011...

with the names "X by Y", which can be read as "one quarter wind from X toward Y", where X is one of the eight principal winds and Y is one of the two adjacent...

(2011-05-10). "Colder and Hotter: Interferometric imaging of {\beta} Cassiopeiae and {\alpha} Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105...