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David Whysong wrote:
Sorry to chime in late, but I haven't been monitoring SAA regularly. Martin Brown wrote: In message m, Jeremiah J. Burton writes What would a quasar look like up close? 3C273 and M87 are about as good targets as any to give a rough idea. M87 isn't a quasar at all, it's a nonthermal radio galaxy. In any case, Sag A* (the black hole at the center of our Galaxy) isn't huge as such things go, and if it were more active it would probably appear as a type 2 Seyfert rather than an obscured quasar. Mind you, M87 might make a tolerable blazar is seen from about 40 degrees away in the right direction. Trying to fit the jet structure gives a cool example of relativistic effects; planar objects (shocks, for example) moving outward with a relativistic flow wil look more edge-on than they really (i.e. geometrically) are, since the back side is seen at an earlier stage in the flow. This may have once been called a Lorentz rotation. Quasars is sometimes reserved for radio loud quasi-stellar objects. Right, and AFAIK there is only 1 known radio-loud active galaxy with a spiral host. There is also an optical luminosity cutoff for quasars. You rang? Gotta add the new Chandra results one of these days. Sad to say, I just learned that Mike Ledlow, who played a big part in work on the radio-loud spiral 0313-192, died suddenly this week in Colorado. Kinda makes me forget that pesky appendectomy last week. Bill Keel |
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