How do they determine the strength of the magnetic field of a neutron star?
...as their strong magnetic field rotates it induces very long wavelength dipole radiation. We don't observe any of this as at very long wavelength it is absorbed in the ISM.Appropriately modify/apply that reasoning/known physics (re magnetic component-energy of e-m energy/field effects associated with massive spinning/orbiting features as Neut. Stars/BHs), and you will 'get' what I've LONG been pointing out about the type of energy which a binary system are 'radiating away' to account for observed decreasing system mass/orbital period decrease.
Once we realize this known physics explains observations of Hulse-Taylor example
Are you even aware of the (electro-)MAGNETIC FIELD ENERGIES involved in such NS features/dynamics?Once we realize this known physics explains observations of Hulse-Taylor example
But you haven't shown that. What you have there is a hypothesis, you have not shown that it can explain the data. There exist very high quality timing datasets for a few binary pulsars, I suggest you try to build a self-consistent model before making any bold claims.
I was not aware of the SZ effect, thanks IMP-9.You weren't aware of a LOT of important relevant astronomical/cosmological KNOWN science facts and understandings. Which is why your obviously 'emotional' cheap shots at me fall flat on your own ignorance/misunderstandings. About time you started to listen instead of ignore, deny and insult etc, isn't it, mate?GR has been shown to fit this the Hulse-Taylor binary to about 2 parts in a thousand
Enough accuracy to convince any knowledgeable, psychologically stable person.
HannesAlfven
Jun 21, 2016Re: "For me the most interesting question is, why is this the only magnetar with a nebula?"
The mystery is slightly lessened once the features of laboratory plasmas are considered: The plasma only glows given a particular charge density. Further, the event is likely not as rare as theorists here assume, as they've yet to consider instances where nebulae are currently thought to be illuminated by sunlight striking gas.
As observations of nebulae improve, it will become apparent that nebulae are composed of plasma filaments which can enter the plasma glow mode.