The conventional colour description takes into account only the peak of the stellar spectrum. In actuality, however, stars radiate in all parts of the spectrum. Because all spectral colours combined appear white, the actual … 詳細

The reason for the odd arrangement of letters in the Harvard classification is historical, having evolved from the earlier Secchi classes and been … 詳細

A number of new spectral types have been taken into use from newly discovered types of stars.
Hot blue emission star classes
Spectra of some very hot and bluish stars exhibit marked emission lines from carbon or nitrogen, or … 詳細

Several spectral types, all previously used for non-standard stars in the mid-20th century, have been replaced during revisions of the stellar … 詳細

The modern classification system is known as the Morgan–Keenan (MK) classification. Each star is assigned a spectral class (from the … 詳細

The stellar classification system is taxonomic, based on type specimens, similar to classification of species in biology: The categories are defined by one or more standard stars for each category and sub-category, with an associated description of the … 詳細

Stellar remnants are objects associated with the death of stars. Included in the category are white dwarfs, and as can be seen from the radically … 詳細