Search results
Appearance
There is a page named "19 Cephei" on Wikipedia
- 19 Cephei is a supergiant star in the northern circumpolar constellation of Cepheus. It has a spectral class of O9 and is a member of Cep OB2, an OB association...8 KB (655 words) - 00:37, 21 August 2024
- Gamma Cephei (γ Cephei, abbreviated Gamma Cep, γ Cep) is a binary star system approximately 45 light-years away in the northern constellation of Cepheus...20 KB (1,809 words) - 18:53, 14 March 2025
- Mu Cephei (Latinized from μ Cephei, abbreviated Mu Cep or μ Cep), also known as the Garnet Star, is a red supergiant star in the constellation Cepheus...26 KB (2,519 words) - 21:47, 15 March 2025
- asterism consisting of α Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Xi Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese...16 KB (1,315 words) - 06:46, 29 January 2025
- VV Cephei, also known as HD 208816, is an eclipsing binary star system located in the constellation Cepheus. It is both a B[e] star and shell star. As...26 KB (2,762 words) - 22:42, 15 March 2025
- Cepheus (constellation) (redirect from Cephei)hypergiant, together with the red supergiants Mu Cephei, MY Cephei, VV Cephei, V381 Cephei, and V354 Cephei are among the largest stars known. In addition...21 KB (2,288 words) - 01:10, 3 March 2025
- Beta Cephei (β Cephei, abbreviated Beta Cep, β Cep) is a triple star system of the third magnitude in the constellation of Cepheus. Based on parallax measurements...17 KB (1,417 words) - 22:09, 22 August 2024
- Delta Cephei (δ Cep, δ Cephei) is a quadruple star system located approximately 887 light-years away in the northern constellation of Cepheus, the King...21 KB (1,806 words) - 19:29, 2 March 2025
- List of largest stars (redirect from SW Cephei)Jeffrey L.; Bennett, Philip D.; Pollmann, Ernst (2015). "VV Cephei Eclipse Campaign 2017/19". The Society for Astronomical Sciences 34th Annual Symposium...254 KB (10,937 words) - 22:40, 19 March 2025
- Classification of a and F Stars", Astrophysical Journal Supplement, 19: 281, Bibcode:1970ApJS...19..281B, doi:10.1086/190209. Frost, E. B. (December 1924), "Fourteen...11 KB (172 words) - 13:48, 15 January 2025
- Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations...27 KB (1,961 words) - 14:46, 17 July 2024
- AR Cephei (AR Cep) is a variable star in the constellation Cepheus. It is classified as a semiregular star with a spectral type of M4III. Aernout de Sitter...4 KB (270 words) - 21:48, 19 March 2025
- S Cephei (S Cep), also designated as HD 206362, is a carbon star and Mira-type variable in the constellation Cepheus. Based on the measurement of its annual...4 KB (306 words) - 22:05, 19 March 2025
- asterism consisting of Xi Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Alpha Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese...12 KB (948 words) - 17:51, 20 October 2024
- S2CID 118403321. McClure, Bruce; Byrd, Deborah (22 September 2021). "Gamma Cephei, aka Errai, a future North Star". earthsky.org. Retrieved 25 December 2021...176 KB (7,772 words) - 06:05, 14 March 2025
- consisting of η Cephei, 4 Cephei, HD 194298, θ Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei. Consequently, the Chinese name for η Cephei itself...12 KB (1,042 words) - 20:11, 27 February 2025
- Spica (category Beta Cephei variables)their spectra. The primary is a blue giant and a variable star of the Beta Cephei type. Spica, along with Arcturus and Denebola—or Regulus, depending on the...26 KB (2,448 words) - 11:26, 19 December 2024
- Beta Centauri (category Beta Cephei variables)the detection of pulsations, the Aa component has been classified as a β Cephei variable. Beta Centauri is well known in the Southern Hemisphere as the...20 KB (1,728 words) - 21:37, 10 March 2025
- Assyrian celestial divination. Carsten Niebuhr Institute Publications. Vol. 19. Museum Tusculanum Press. p. 163. ISBN 978-87-7289-287-0. Coleman, Leslie...148 KB (16,400 words) - 19:36, 19 March 2025
- classification of B1 V. It is a Beta Cephei variable, ranging from 5.01 to 4.96 magnitude with a period of 0.19 days. Closer examination shows there are...8 KB (641 words) - 17:14, 16 July 2024
- discoveries of the variability respectively of β Lyræ and of δ Cephei dated from 10 Sept. and 19 Oct. 1784 (ib. lxxv. 153, lxxvi. 48). He perceived the double
- w:Earth. The spatial dimension of this cluster is about 19 w:light years across. A Delta Cephei type w:variable star designated U Sagittarii is a member