Reinvestigation of the unified theory for Seyfert galaxies by observing water vapor masers
| Project/Area Number |
17340052
|
|---|
| Research Category |
Grant-in-Aid for Scientific Research (B)
|
| Allocation Type | Single-year Grants |
|---|
| Section | 一般 |
|---|
| Research Field |
Astronomy
|
|---|
| Research Institution | University of Tsukuba |
|---|
Principal Investigator |
NAKA Naomasa University of Tsukuba, Graduate School of Pure and Applied Sciences, Professor (80192665)
|
|---|
| Project Period (FY) |
2005 – 2007
|
| Project Status |
Completed (Fiscal Year 2007)
|
| Budget Amount *help |
¥14,100,000 (Direct Cost: ¥13,800,000、Indirect Cost: ¥300,000)
Fiscal Year 2007: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2006: ¥1,000,000 (Direct Cost: ¥1,000,000)
Fiscal Year 2005: ¥11,800,000 (Direct Cost: ¥11,800,000)
|
|---|
| Keywords | astronomical observations / radio astonomy / radio telescopes / galaxies / active galactic nuclei / black holes / メーザー / 銀河形成進化 / 宇宙物理 / 宇宙論 / 宇宙メーザー / セイファート銀河 |
|---|
| Research Abstract |
(1) The 20-GHz band observing system of the Tsukuba 32-m telescope of the Geographical Survey Institute was newly constructed to make observations of water-vapor maser emission in the nuclear regions of Seyfert galaxies. The HPBW of the telescope was 100" at 22 GHz, and the main beam efficiency and the aperture efficiency were 0.52 and 0.40, respectively The receiver frontend was a HEMT amplifier cooled at 20 K and had sensitivity at the radio frequencies of 19.5 - 25.2 GHz. The intermediate frequencies were 4 - 8 GHz. A spectrometer was the Fourier transformation-type digital spectrometer with the frequency band of 1 GHz and the channel number of 16 k. The system noise temperature including the atmosphere and ohmic loss was 60-80 K at the zenith. The system is useful to study the nuclear regions of Seyfert galaxies by observing water-vapor maser emission.
(2) We started monitoring observations of velocities of water masers from Seyfert galaxies. In addition, we revealed that a maser disk at the center of a type 2 Seyfert, IC 1481, was thick and massive, confirming our hypothesis in which the difference between the type 1 and 2 of Seyfert galaxies is caused by not only the viewing angle of the accretion disk but also the thickness of the disk.
|
Report
(4 results)
Research Products
(33 results)
-
-
-
-
-
[Journal Article] Water-Vapor Maser Survey for Active Galactic Nuclei : A Megamser in NGC 69262005
Author(s)
Sato,N., Yamauchi, A., Ishihara,Y., Sorai,K., Kuno,N., Nakai,N., Balasubramanyam, R., Hall, P.
-
Journal Title
Publication of the Astronomical Journal of Japan 57
Pages: 587-594
Description
「研究成果報告書概要(欧文)」より
Related Report
-
-
-
-
[Journal Article] Water-Vapor Maser Survey for Active Galactic Nuclei : A Megamaser in NGC 69262005
Author(s)
Sato, N., Yamauchi, A., Ishihara, Y., Sorai, K., Kuno, N., Nakai, N., Balasubramanyam, R., Hall, P.
-
Journal Title
Publications of the Astronomical Society of Japan 57
Pages: 587-587
NAID
Related Report
-
[Journal Article] High Angular Resolution Observations of the (J, K) = (1,1), (2,2), and (3,3) Transitions of Ammonia in NGC 2532005
Author(s)
Takano, S., Hofner, P., Winnewisser, G., Nakai, N., Kawaguchi, K.
-
Journal Title
Publications of the Astronomical Society of Japan 57
Pages: 549-549
NAID
Related Report
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
-
