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Дата изменения: Mon Oct 16 15:45:11 2000 Дата индексирования: Mon Oct 1 22:36:56 2012 Кодировка: Поисковые слова: massive stars |
Comment on J1232-0224
Hooimeyer et al (1992a) detected the source on the Green Bank-Owens Valley baseline at 5 GHz (correlated flux density 180 mJy) and found that the nuclear emission was probably diffuse. The jet position angle in a 1.4 GHz VLA image (Hintzen, Ulvestad & Owen 1983) is similar to that in our VLBA image. Our image is consistent with the images at 2.3 and 8.4 GHz from the VLBA Calibrators database.