Centaurus A | |
M87 jet turns into intense radio source |
Cygnus A appears to be double galaxy with radio emission coming from distant lobes | |
Brightest radio object in sky: took a long time to find optical counterpart, since it is a distant galaxy. Emission is synchrotron from electrons ejected from centre
Note jet |
Nowhere near largest radio source! |
Position of 3C273 found v. accurately by lunar occultation, so could be identified with 13 mag. blue "star" with jet projecting from it | |
This shows the problem: it shows a galaxy (maybe 2) a quasar and a star. Which is which? | Credit: C. Steidel (Caltech), HST, NASA |
3C 273 bright enough that it had been recorded on old plates: hadn't moved in sky, so must be distant. |
i.e. light output occurs from same size region as supergiant star, but energy ∼ 1010 larger |
Best Bet Model! Supermassive black hole, consuming 10-20 M₀/year Surrounding galaxy produces emission lines "Flickering" from stars falling into black hole |
Hence expect following scenario:
Quasars very plentiful in early universe. We see Seyfert galaxies, which seem to be intermediate, so quasars evolve to Seyferts or radio galaxies as black hole consumes most of central core, and then to normal spiral as central core becomes used up |
About 10000 quasars known, and each is very characteristic: red-shifts and spectrum are very distinct.
However several pairs which lie very close in sky: e.g. 0957 +561A & 0957 +561B are 6" apart in sky and have identical red-shifts. Note "fuzz" sticking out of lower one |
Can be understood via radio image: massive galaxies will bend light |
THis one is imaged 4 times (the Einstein cross) Can just see the galaxy | Credit & Copyright: J. Rhoads (STScI) et al., WIYN, AURA, NOAO, NSF |
Should allow us to measure mass of intervening galaxy, but not easy in practice.
And finally amongst the wierdos
Found originally by Vela satellite (designed to look for γ's from nuclear explosions). Can identify source by using timinng with various satellites Bursts last 1/10 - 100s, no particular pattern |
Problems: Could not be identified with any known object
Possibly collisions between stars in very distant galaxies, or some unusual form of supernova | Image Credit: S. Kulkarni, J. Bloom, P. Price, Caltech - NRAO GRB Collaboration |