RW Cephei is a K-type hypergiant and a semirregular variable star in the constellation Cepheus, at the edge of the Sharpless 132 H II region and close...

Alpha Cephei, with an apparent magnitude of 2.5. Delta Cephei is the prototype of an important class of star known as a Cepheid variable. RW Cephei, an...

Robin Wight, botanist, noted as R.W. RW is the designation for the 15th variable star named in a constellation: RW Cephei, an orange hypergiant located...

Köhler, Rainer (September 2024). "Time Evolution Images of the Hypergiant RW Cephei during the Rebrightening Phase Following the Great Dimming". The Astrophysical...

Köhler, Rainer (September 2024). "Time Evolution Images of the Hypergiant RW Cephei during the Rebrightening Phase Following the Great Dimming". The Astrophysical...

mass-loss, similar to those of Betelgeuse and RW Cephei. The rebrightening of B90, just like RW Cephei, took twice as long as that of Betelgeuse which...

In 2022, the array was used to observe the disc of the hypergiant star RW Cephei during its ongoing dimming event. CHARA holds annual science meetings...

Humphreys, Roberta (2023-05-11). "The recent mass-loss history of the hypergiant RW Cep". Research Notes of the American Astronomical Society. 7 (5): 92. Bibcode:2023RNAAS...

bound, yellow hypergiants and red supergiants are not clearly separated; RW Cephei (roughly 4,000 K (3,730 °C; 6,740 °F), 295,000 L☉) is an example of a...

There are also giant K-type stars, which range from hypergiants like RW Cephei, to giants and supergiants, such as Arcturus, whereas orange dwarfs, like...