1. Upper limit of 3.3 astronomical units to the diameter of the galactic center radio source Sgr A*
- Author
-
Backer, D.C., Zensus, J.A., Kellermann, K.I., Reid, M., Moran, J.M., and Lo, K.Y.
- Subjects
Radio sources (Astronomy) -- Observations ,Galactic center -- Observations ,Science and technology ,Observations - Abstract
Sagittarius (Sgr) A* is a unique radio source located at the center of our galaxy. The radiation from Sgr A* may be generated in matter accreting onto a massive black hole. In observations at long wavelengths, the apparent angular size of Sgr A* decreases in the manner expected for emission from a point source scattered by electron density fluctuations along the line of sight. Measurements at a wavelength of 7 millimeters with the nearly completed Very Long Baseline Array indicate a size of 0.7 milliarc seconds, which is consistent with an extrapolation from results at longer wavelengths. The true size of Sgr A* must be less than 0.4 milliarc seconds, or 3.3 astronomical units. The inferred black hole mass is less than 1.5 x [10.sup.6] solar masses according to a recent model for the emission., Sagittarius A* is an enigmatic object. Recent speckle imaging at a wavelength (λ) of 2 μm indicates that the centroid of the stellar sources at the galactic center is much [...]
- Published
- 1993