G'day Modest
You said:
Quote:
|
I should tell you, Pluto. If you want to continue criticizing other people's positions (which are well-backed by evidence and theory) with your own strange claims then you need to do better than "you get this feeling If you know what I mean".
|
You are miss understanding my position.
I do not have a position.
I keep on telling you that it will take me at least two more years of reading to undertsand the workings of the parts.
I have read your links and I find limited in information.
My aim is to understand the actual trigger that starts the jets.
So far all the papers that I have read talk around the subject. They are getting closer, but! they are limited by the tools that they are using.
In the last 12 mths, the papers have become better.
If you do not want me to share the links that I'm reading, thats fine.
It has been Xmas break and time has been limted so please do not expect answers that most scientists do not even know about.
Do you actually read the links?
If you have read the links than you have read them out of context when they write about compact matter.
What do you think is the main body that plays the main part?
The transition phase is the key.
This is not a new topic, Wheeler in 1996 wrote this paper.
[astro-ph/9606119] Black Hole X-ray Transients
Black Hole X-ray Transients
Authors: J. Craig Wheeler (Dept. of Astronomy, U. of Texas)
(Submitted on 19 Jun 1996)
Quote:
|
Abstract: The observations and theory of the exciting new class of galactic black hole X-ray transients is reviewed. Seven of these systems have measured mass functions or mass estimates in excess of stable neutron stars, making them excellent black hole candidates. Two of them have revealed ``superluminal" radio jets. Study of the hard and soft radiation from these sources has given tight constraints on the physics of the viscosity of the accretion disk and promises firm proof that these systems contain black holes. This will allow us to search for black holes of more moderate mass and apply the knowledge of these systems to suspected supermassive black holes in AGN's. The most plausible mechanism for triggering the outburst of black hole candidate X-ray transients is the ionization thermal instability. The disk instability models can give the deduced mass flow in quiescence, but not the X-ray spectrum. Advection models that can account for the quiescent X-ray spectrum are difficult to match with the non-steady state, quiescent Keplerian disks. Self-irradiation of the disk in outburst may not lead to X-ray reprocessing as the dominant source of optical light, but may play a role in the ``reflare." The hard power-law spectrum and radio bursts may be non-thermal processes driven by the flow of pair--rich plasma from the disk at early times and due to the formation of a pair--rich plasma corona at late times. The repeated outbursts in systems like GRO J0422+32 suggest some sort of clock, but it is unlikely that it has anything to do with a simple X-ray heating of the companion star. These systems typically have low mass secondaries and their evolutionary origin is still mysterious.
|
Research into these area is moss important.
and yet the key issue in the formation of the jet has not been resolved. There are a number of theories and experiments on Z-pinch explaining the formation of jets and the resultant formation of Neutrons and their ultra compaction.
I stll have a month or more of reading on this subject.
I'm not interested in feeling right, I just want to know and understand. So I thank you for your time.
