Abstract
We report the first detection of a water megamaser in a radio-loud galaxy, 3C 403, and present a follow-up study using the VLA. 3C 403 has been observed as a part of a small sample of FR II galaxies with evidence of nuclear obscuration. The isotropic luminosity of the maser is ∼1200 Lʘ. With a recessional velocity of cz ∼- 17680 km s−1 it is the most distant water maser so far reported. The line arises from the densest (>108 cm −3) interstellar gas component ever observed in a radio-loud galaxy. Two spectral features are identified, likely bracketing the systemic velocity of the galaxy. Our interferometric data clearly indicate that these arise from a location within 0.1″ (≈110 pc) from the active galactic nucleus. We conclude that the maser spots are most likely associated with the tangentially seen parts of a nuclear accretion disk, while an association with dense warm gas interacting with the radio jets cannot yet be ruled out entirely.
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Tarchi, A., Henkel, C., Chiaberge, M., Menten, K.M., Brunthaler, A., Moscadelli, L. (2005). Probing the Obscuring Medium Around Active Nuclei Using Masers: The Case of 3C 403. In: Baan, W., Hagiwara, Y., van Langevelde, H. (eds) Dense Molecular Gas Around Protostars and in Galactic Nuclei. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3831-3_14
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DOI: https://doi.org/10.1007/1-4020-3831-3_14
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