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
Redshift | Parsecs /Distance | Lightyears /Lookback Years | | |
~0 | 29pc | 94ly | | Algol |
|
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)
Index