[net.physics] pulsing large objects

MJackson.Wbst@XEROX.ARPA (06/12/84)

	"I mentioned before that a giant lens could cause the appearance 
	of a (light-year-wide) simultaneous flash (ie, a light-year-wide
	glass lens) for an observer in a particular position.  Does anybody 
	know if the same could be true of a gravitational "lens"?
	--JoSH"

No reason why not; if the gravitational "lens" is producing more than
one apparent object, *and if the path lengths/light travel time are the
same*, the separated images would appear to flash together.  This would
only be true for a *very* specific set of positions, of course.

Mark

JoSH@RUTGERS.ARPA (06/25/84)

From:  JoSH <JoSH@RUTGERS.ARPA>

I mentioned before that a giant lens could cause the appearance 
of a (light-year-wide) simultaneous flash (ie, a light-year-wide
glass lens) for an observer in a particular position.  Does anybody 
know if the same could be true of a gravitational "lens"?
--JoSH
-------

gary@mit-eddie.UUCP (Gary Samad) (06/30/84)

><

What are the observed periods of quasars?  How big were quasars expected
to be?

	G~

allan@noao.UUCP (07/02/84)

  One of the problems with interpreting quasars' light curves is that they are
not periodic. The best that you can do is give a typical time for a quasars
to vary by a significant amount. This time goes from about an hour upto several
years depending on the individual object. The expected timescale for variations
depends on what model you believe in. The favourite model consists of an
accretion disk around a black hole, in which case the quasar cannot vary
faster than the light travel time across the black hole (unless relativistic
beaming is important).

  Part of the problem in measuring quasar variability is that most quasars 
are not very variable. Here at Kitt Peak, Bill Keel and I are trying to measure
the variability of a (hopefully) unbiased sample of quasars. We can detect 
variation as small as 0.05 magnitudes (5 percent for you non astronomers).
The project is going fairly well and a few more observing runs should complete
the data acquisition.


Peter (theories to go) Allan
Kitt Peak National Observatory
Tucson, Az
UUCP:	{akgua,allegra,arizona,decvax,hao,ihnp4,lbl-csam,seismo}!noao!allan
ARPA:	noao!allan@lbl-csam.arpa