Similarities between Gamma Cephei and IAU Working Group on Star Names
Gamma Cephei and IAU Working Group on Star Names have 4 things in common (in Unionpedia): Bayer designation, Bright Star Catalogue, International Astronomical Union, Iota Draconis.
Bayer designation
A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name.
Bayer designation and Gamma Cephei · Bayer designation and IAU Working Group on Star Names ·
Bright Star Catalogue
The Bright Star Catalogue, also known as the Yale Catalogue of Bright Stars or Yale Bright Star Catalogue, is a star catalogue that lists all stars of stellar magnitude 6.5 or brighter, which is roughly every star visible to the naked eye from Earth.
Bright Star Catalogue and Gamma Cephei · Bright Star Catalogue and IAU Working Group on Star Names ·
International Astronomical Union
The International Astronomical Union (IAU; Union astronomique internationale, UAI) is an international association of professional astronomers, at the PhD level and beyond, active in professional research and education in astronomy.
Gamma Cephei and International Astronomical Union · IAU Working Group on Star Names and International Astronomical Union ·
Iota Draconis
Iota Draconis (ι Draconis, abbreviated Iota Dra, ι Dra), also named Edasich, is a star in the northern circumpolar constellation of Draco.
Gamma Cephei and Iota Draconis · IAU Working Group on Star Names and Iota Draconis ·
The list above answers the following questions
- What Gamma Cephei and IAU Working Group on Star Names have in common
- What are the similarities between Gamma Cephei and IAU Working Group on Star Names
Gamma Cephei and IAU Working Group on Star Names Comparison
Gamma Cephei has 57 relations, while IAU Working Group on Star Names has 29. As they have in common 4, the Jaccard index is 4.65% = 4 / (57 + 29).
References
This article shows the relationship between Gamma Cephei and IAU Working Group on Star Names. To access each article from which the information was extracted, please visit: