As it has very strong and abnormal radiation, the external OH megamaser attracts many people. A lot of work has been done in searching for extragalactic OH megamaser and some observations of VLA-A, MERLIN and VLBI wer...As it has very strong and abnormal radiation, the external OH megamaser attracts many people. A lot of work has been done in searching for extragalactic OH megamaser and some observations of VLA-A, MERLIN and VLBI were conducted for the extragalactic OH megamaser galaxies which had been observed with single-antenna, e. g.展开更多
ⅢZw35 is an external OH megamaser galaxy. Staveley-Smith et al. observedit using single-dish. Chapman et al.studied it through combined optical, infrared and ra-dio observation. Montgomery and Cohen observed the OH m...ⅢZw35 is an external OH megamaser galaxy. Staveley-Smith et al. observedit using single-dish. Chapman et al.studied it through combined optical, infrared and ra-dio observation. Montgomery and Cohen observed the OH megamaser radiation ofⅢZW35 using MERLIN. The present author fitted the radiation spectrum observed byStaveley-Smith et al. in ref.[4].In this note we make a further investigation on the posi-展开更多
基金Project supported by Radio Astronomy Union Laboratory, Academia Sinica
文摘As it has very strong and abnormal radiation, the external OH megamaser attracts many people. A lot of work has been done in searching for extragalactic OH megamaser and some observations of VLA-A, MERLIN and VLBI were conducted for the extragalactic OH megamaser galaxies which had been observed with single-antenna, e. g.
基金Project supported by the National Natural Science Foundation of China and Radio Astronomy Union Laboratory of Chinese Academy of Sciences.
文摘ⅢZw35 is an external OH megamaser galaxy. Staveley-Smith et al. observedit using single-dish. Chapman et al.studied it through combined optical, infrared and ra-dio observation. Montgomery and Cohen observed the OH megamaser radiation ofⅢZW35 using MERLIN. The present author fitted the radiation spectrum observed byStaveley-Smith et al. in ref.[4].In this note we make a further investigation on the posi-