€Model introduced by Wu
et al (2002) to deal with absence of polarisation and emission lines in
RXJ1914.4+2457
€
€Scaled-up version of Jupiter-moon interactions
heating Jupiter¹s
atmosphere at footpoints of magnetic field lines threading moon, BUT:
a)energy release boosted
by stronger magnetic field
b)shorter period
c)secondary larger than a
moon
d)
€Up to 1036 ergs/s available (depending on degree of
asynchronism)
€
€Star shines by electrical
resistive heating:
new
mechanism
after
1.nuclear fusion
2.accretion
3.magnetic
(magnetars)
4.