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There is a page named "Gamma Doradus" on Wikipedia
- Gamma Doradus, Latinized from γ Doradus, is the third-brightest star in the southern constellation of Dorado. It is faintly visible to the naked eye with...13 KB (749 words) - 22:41, 17 July 2024
- Gamma Doradus variables are variable stars which display variations in luminosity due to non-radial pulsations of their surface. The stars are typically...22 KB (1,494 words) - 22:42, 17 July 2024
- blocking and is believed to drive pulsations in the γ {\displaystyle \gamma } Doradus variables. Observations from the Kepler satellite revealed eccentric...18 KB (2,290 words) - 07:53, 18 March 2025
- Variable star (section Gamma Doradus variables)Deneb, in the constellation of Cygnus is the prototype of this class. Gamma Doradus (γ Dor) variables are non-radially pulsating main-sequence stars of...51 KB (6,578 words) - 21:15, 15 March 2025
- HR 8799 (category Gamma Doradus variables)whose orbital motion was confirmed by direct imaging. The star is a Gamma Doradus variable: its luminosity changes because of non-radial pulsations of...46 KB (4,295 words) - 19:44, 8 February 2025
- one rotating ellipsoidal variable, seven Delta Scuti variables, six Gamma Doradus variables, and one hybrid δ Sct/γ Dor pulsator. Four spectroscopic binary...8 KB (710 words) - 11:06, 18 July 2024
- HD 49434 (category Gamma Doradus variables)is a Gamma Doradus variable. Observation of the star during the CoRoT mission showed ten pulsation frequencies, four of which are typical for Gamma Doradus...11 KB (751 words) - 22:31, 14 September 2024
- QW Puppis (category Gamma Doradus variables)it is approximately 69.5 light years away based on parallax. It is a Gamma Doradus variable, ranging from 4.5 to 4.47 magnitude with a period of 0.96 days...6 KB (425 words) - 22:00, 9 November 2022
- variable stars, including the measurement of the two sinusoidal periods of Gamma Doradus. The UBV photometric system for measuring stellar fluxes he devised...10 KB (957 words) - 06:10, 21 January 2022
- HD 149989 (category Gamma Doradus variables)et al. sifted through that list, and determined that HD 149989 is a Gamma Doradus type star. It has a period of 0.42658 days. It was given its variable...9 KB (690 words) - 00:06, 31 December 2024
- yellow-white stars which orbit each other every 39.88 days. The primary is a Gamma Doradus variable, pulsating over a period of 1.45 days. The fainter star is...33 KB (3,326 words) - 01:39, 28 February 2025
- B stars, one being a Delta (δ) Scuti variable, and three candidate Gamma Doradus (γ Dor) variables. There may also be three Be stars. The core of the...7 KB (624 words) - 07:00, 23 August 2024
- 9 Aurigae (category Gamma Doradus variables)discovered that the star is a variable star in 1990. It is a well-studied Gamma Doradus variable, and was one of the first stars to be so-classified. This star...12 KB (1,375 words) - 13:40, 16 March 2025
- de Données astronomiques de Strasbourg. Retrieved 24 October 2013. Gamma Doradus Stars: Defining a New Class of Pulsating Variables, Anthony B. Kaye...35 KB (1,751 words) - 14:07, 20 March 2025
- variables displaying characteristic frequencies of both Delta Scuti and Gamma Doradus variables. On the Hertzsprung–Russell diagram, these stars are positioned...165 KB (18,999 words) - 20:29, 19 March 2025
- suggests it is either a spectroscopic binary or (more likely) a pulsating Gamma Doradus-type variable. If the latter is the case, it is estimated to be 1.39...51 KB (6,172 words) - 23:25, 1 March 2025
- Iota Trianguli Australis (category Gamma Doradus variables)member, component A, is yellow-white hued F-type subgiant star and a Gamma Doradus type variable, pulsating by 0.12 magnitudes with a dominant period of...9 KB (603 words) - 05:35, 21 August 2024
- suggests it is either a spectroscopic binary or (more likely) a pulsating Gamma Doradus-type variable. Alchiba has 32% more mass and is 37% larger than the...11 KB (966 words) - 01:28, 25 January 2025
- 19 Aquilae (category Gamma Doradus variables)subgiant to a giant stage. Poretti et al. (2003) list it as a suspected Gamma Doradus variable, and it is located near the cooler end of the instability strip...9 KB (681 words) - 11:23, 22 August 2024