Individual sheet: xi Per

ID: xi Per

Simbad
Other ID: HD24912
RA (J2000): 03 58 57.90
DEC (J2000): +35 47 27.71

Spectral type(s): O7.5III (or I)

Multiplicity:
Undetermined multiplicity
Period(s): /
Orbital solution: /
Ref: /

Comments:
The potential non-thermal radio emission reported by Schnerr et al. (2007) might be attributed to a bow-shock between the stellar wind and the interstellar material, as this object is a runaway star.

Home List B Bibliography