Water-vapor maser disk at the nucleus of the Seyfert 2 IC 2560
Abstract
We observed the H2O maser at the nucleus of the Seyfert 2, IC 2560, using the VLBA and the phased VLA. The systemic, red-shifted and blue-shifted maser features and a continuum component have been detected. We propose a maser disk in the nuclear region. The systemic and red-shifted features are emitted from a nearly edge-on disk with the position angle of PA = −47°. The thickness is 2H < 0.025 pc. The binding mass is 3.5 × 106M⊙. Assuming the Keplerian rotation, the radii at the disk are r = 0.087-0.335 pc and the rotation velocities are 213-418 km s−1. The mean density within the inner radius is 1.3 × 109M⊙ pc−3, suggesting a massive black hole at the center. A continuum component is considered as a jet ejected from the nucleus, with an angle of 70° from the disk. The blue-shifted maser feature is located on the continuum component, being interpreted to be a `jet maser'.
- Publication:
-
Astrophysical Masers and their Environments
- Pub Date:
- March 2007
- DOI:
- Bibcode:
- 2007IAUS..242..412Y
- Keywords:
-
- galaxies:active;
- galaxies:individual (IC 2560);
- galaxies:nuclei;
- galaxies: Seyfert