Astrophysics (Index)About

Be star

(early star with Balmer emission lines)

The term Be star indicates a B-type star with emission lines (as per the spectral type suffix "e"), but is commonly used to indicate those with a particular frequent underlying cause: hydrogen emission lines presumed to stem from rapid rotation, producing a circumstellar disk of gas ejected by the rotation (a decretion disk), and heating it to produce Balmer series emission lines. They often show overlaid H-alpha emission and absorption lines, each with considerable line broadening, the former indicating the rotation of the disk and the latter, the rotation of the star. The term classical Be star is used to distinguish this from those with other characteristics, presumed to be formed by some other mechanism. The term Be star is now so commonly associated with the rapidly rotating type that such rotating A-type stars and O-type stars are sometimes referred to as Be stars.

The term B[e] star specifically indicates forbidden emission lines, suggesting some difference in the underlying cause or some additional factor.


(star type,Balmer series,rotation)
Further reading:
https://en.wikipedia.org/wiki/Be_star
https://en.wikipedia.org/wiki/B(e)_star
http://www.astrosurf.com/buil/us/bestar.htm
https://www-n.oca.eu/stee/page1/page3/page3.html

Referenced by pages:
binary star
chemically peculiar star (CP star)
decretion disk
emission-line star
LB-1
shell star (sh)

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