Infrared observations and a model of beta Per.
Abstract
Infrared light curves of fi Per are presented for wavelengths of , , and . From these are deduced a model of the system which has a gas stream flowing from the Ko star to the B8 star. Its temperature and electron density vary from 5 to 20 x I0 K and 30 to 5 x 1011 cm-3 respectively. The mass transfer rate is I 8 x I0- M0!yr.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- November 1975
- DOI:
- 10.1093/mnras/173.2.271
- Bibcode:
- 1975MNRAS.173..271L