Imaging the Accretion Flow Around the Black Hole SgrA*                                                                        

Images of the accretion flow around a non-rotating (left) and rapidly rotating (right) black hole. Superposed on these images is the lensed equatorial coordinate grid. You may enlarge each photo by clicking on it.

  Below are links to two movies that illustrate the appearance of a hot spot in orbit around the black hole at the center of the Milky-Way galaxy. In each movie, the frame on the left shows the image of the spot as it moves around the black hole in a circular orbit of a radius that is only three times larger than the horizon size for a non-spinning black hole (r=6GM/c^2). The scales of this frame are in units of micro-arcseconds. The accretion disk (in which the hot spot is embedded) is viewed at an angle of 45 degrees. The tick marks reflect the orientation of the observed polarization. The frame on the right shows the polarized flux (upper panel) and the fractional flux (lower panel) as they evolve during the orbit of the hot spot. The difference between the two movies is that one shows the case of a non-spinning black hole and the second shows the case of a maximally spinning black hole. At present, we do not know the rate by which the black hole in the Galactic center is spinning. Future observations of such images will be able to infer the spin of the black hole, as well as test the validity of Einstein's theory of gravity.          For more details about the parameters of the calculation, click on Broderick & Loeb, astro-ph/0509237                                                                                                                                                                                                              Movies can be played with QuickTime. If you have difficulties opening the files directly: (i) Save the files on your computer; (ii) Start up QuickTime from the start-->program menu; (iii) Choose the file-->open option and open the file from QuickTime; (iv) QuickTime may ask if you wish to convert the file to a QuickTime format - Choose yes; (v) Select `Loop' out of the `Movie' entry on the upper bar of QuickTime; (vi) Play the movie.                                         
Movie 1: Non-spinning Black Hole
Movie 2: Maximally-spinning Black Hole Related papers:                                          Broderick & Loeb astro-ph/0506433                                          astro-ph/0508386                                          astro-ph/0509237