Astrophysics (Index)About

Algol

(Beta Per, β Per, Beta Persei, β Persei)
(a multiple-star system demonstrating effects of mass transfer)

Algol (Beta Persei, β Persei, Beta Per, or β Per) is a triple star system including an eclipsing spectroscopic binary, and whose stars show characteristics that do not fit within normal main-sequence evolution, which is presumed to be a consequence of mass transfer between stars. Characteristics (β Per Aa1):

The existence of the abnormal stellar characteristics (ascribed to mass transfer) is termed the Algol paradox.


The terms Algol variable (or just Algol) is a class of variable stars for which Algol is the prototype.


(star,binary star,variable star)
Further reading:
https://en.wikipedia.org/wiki/Algol
https://en.wikipedia.org/wiki/Algol_variable
http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=algol
https://www.aavso.org/vsots_betaper
RedshiftParsecs
/Distance
Lightyears
/Lookback Years
  
~029pc94lyAlgol
Coordinates:Beta Per
J030810.13245+405720.3280

Referenced by pages:
B-type star (B)
binary star
mass transfer
post-common-envelope binary (PCEB)
variable star
Vogt-Russell theorem (VR theorem)

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