A high-resolution study of SGR-B2 at CM-wavelengths |
| |
Authors: | T B Pyatunina |
| |
Institution: | (1) Special Astrophysical Observatory, USSR Academy of Sciences, Leningrad, Pulkovo, U.S.S.R. |
| |
Abstract: | The radio source Sgr-B2 was studied with the radio telescope of the USSR Academy of Sciences, RATAN-600, at wavelengths 13, 8.2, 3.9, 2.08, and 1.38 cm. The brightness distributions obtained allow us to defined spectra of individual components and to revise a total spectrum of the source itself. It was shown that the source contains no less than four ultracompact details with electron densities exceeding 2×104 cm–3. An extended detail with a flux density at 1.38 cm equal to 12.2 f.u. and an angular size 58 arc sec was found in a nuclear region. Excitation parameters of all compact details were shown to correspond to stars of a spectral type earlier than O6 (U 60). A relation (logN
e
–logd) for all Hii regions in the field around Sgr-B2, including G 0.6-0.0 and G 0.5-0.0, was constructed and shown to be nearly linear, with a slope –1.2. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|