Astrophysics (Index)About

star count

(surveys of stars counting them according to some criteria)

A star count is, in effect, an survey (or analysis of existing survey data) counting stars according to some criteria. A motivation for such bookkeeping has been to determine the density of stars, through classifying them by apparent magnitude and making adjustments to accommodate biases that affect the counts, such as the Eddington bias and Malmquist bias. Another motivation is determining the birthrates and lifetimes of different spectral classes.

Analogous counting and analysis is used for other astronomical phenomena, e.g., galaxies, supernovae, and extra-solar planets. Counts of the former two are considered revealing regarding current ideas in cosmology.


(astronomy,stars,surveys)
Further reading:
https://en.wikipedia.org/wiki/Star_count
https://www.oxfordreference.com/display/10.1093/oi/authority.20110803100528472
https://ui.adsabs.harvard.edu/abs/2001AJ....122.1827V/abstract
https://ui.adsabs.harvard.edu/abs/2002ApJ...578..151S/abstract

Referenced by pages:
field star
stellar evolution
Triangulum II (Tri II)

Index