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A Hess diagram plots the relative density of occurrence of stars at differing color–magnitude positions of the Hertzsprung–Russell diagram for a given galaxy or resolved stellar population. The diagram is named after who originated it in 1924. Its use dates back to at least 1948. Hess diagrams are widely used in the study of discrete resolved stellar systems in and around the Milky Way - specifically, in the analysis of globular clusters, satellite galaxies, and stellar streams.

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  • Hess diagram
  • 헤스 다이아그램
  • Diagrama de Hess
  • 赫斯圖
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  • A Hess diagram plots the relative density of occurrence of stars at differing color–magnitude positions of the Hertzsprung–Russell diagram for a given galaxy or resolved stellar population. The diagram is named after who originated it in 1924. Its use dates back to at least 1948. Hess diagrams are widely used in the study of discrete resolved stellar systems in and around the Milky Way - specifically, in the analysis of globular clusters, satellite galaxies, and stellar streams.
  • Um Diagrama de Hess traça a relativa densidade de ocorrência de estrelas em diferentes posições de cor–magnitude do Diagrama de Hertzsprung-Russell para uma dada galáxia. O diagrama é nomeado após , que o originou em 1924. Seu uso remonta a, pelo menos, 1948.
  • 赫斯圖繪出指定星系赫羅圖在不同颜色-星等范围中的恒星密度。 這種圖是由赫斯在1924年命名的。 他使用的年代至少延續至1948年。 右图是利用斯隆数字巡天释放的公开数据绘制的银河系银纬大于80度的恒星的赫斯图,图中用颜色区分赫斯图上的恒星密度。这是常用的天文学研究方法,通常会将来源于观测数据的赫斯图与理论模型进行对比。
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  • A Hess diagram plots the relative density of occurrence of stars at differing color–magnitude positions of the Hertzsprung–Russell diagram for a given galaxy or resolved stellar population. The diagram is named after who originated it in 1924. Its use dates back to at least 1948. Hess diagrams are widely used in the study of discrete resolved stellar systems in and around the Milky Way - specifically, in the analysis of globular clusters, satellite galaxies, and stellar streams.
  • Um Diagrama de Hess traça a relativa densidade de ocorrência de estrelas em diferentes posições de cor–magnitude do Diagrama de Hertzsprung-Russell para uma dada galáxia. O diagrama é nomeado após , que o originou em 1924. Seu uso remonta a, pelo menos, 1948.
  • 赫斯圖繪出指定星系赫羅圖在不同颜色-星等范围中的恒星密度。 這種圖是由赫斯在1924年命名的。 他使用的年代至少延續至1948年。 右图是利用斯隆数字巡天释放的公开数据绘制的银河系银纬大于80度的恒星的赫斯图,图中用颜色区分赫斯图上的恒星密度。这是常用的天文学研究方法,通常会将来源于观测数据的赫斯图与理论模型进行对比。
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