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We present observational results of water vapor maser emission with our high-sensitivity 22 GHz VLBI imaging of the Seyfert galaxy NGC 1068. In this galaxy, there are the following four nuclear radio sources; NE, C, S1, and S2. Among them, the S1 com
Externí odkaz:
http://arxiv.org/abs/2211.02280
Publikováno v:
Publications of the Astronomical Society of Japan. 75:71-81
We present observational results of water vapor maser emission with our high-sensitivity 22 GHz VLBI imaging of the Seyfert galaxy NGC 1068. In this galaxy, there are the following four nuclear radio sources; NE, C, S1, and S2. Among them, the S1 com
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04d0d20e7a2443642c8543d8447465e6
https://doi.org/10.1093/pasj/psac092
https://doi.org/10.1093/pasj/psac092
Publikováno v:
Publications of the Astronomical Society of Japan; Feb2023, Vol. 75 Issue 1, p71-81, 11p