arvau

Wikipedia / Shapley–Sawyer Concentration Class

The Shapley–Sawyer Concentration Class is a classification system on a scale of one to twelve using Roman numerals for globular clusters according to their concentration. The most highly concentrated clusters such as M75 are classified as Class I, with successively diminishing concentrations ranging to Class XII, such as Palomar 12. (The class is sometimes given with numbers [Class 1–12] rather than with Roman numerals.)

From 1927 to 1929, Harlow Shapley and Helen Sawyer Hogg began categorizing clusters according to the degree of concentration the system has toward the core using this scale. This became known as the Shapley–Sawyer Concentration Class.

Classes

Class

Description

Example

High concentration toward the center

Dense central concentration

Strong inner core of stars

Intermediate rich concentrations

Intermediate concentrations

Intermediate mild concentration

Intermediate loose concentration

Rather loosely concentrated towards the center

Loose towards the center

Loose

Very loose towards the center

Almost no concentration towards the center

References