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| Content Provider | Springer Nature Link |
|---|---|
| Author | Zhang, J. S. Wang, J. |
| Copyright Year | 2011 |
| Abstract | H$_{2}$O maser emissions have been found in external galaxies for more than 30 years. Main sciences associated with extragalactic H$_{2}$O masers can be summarized roughly into three parts: maser emission itself, AGN sciences and cosmology exploration. Our work in this field focusses on two projects: X-ray data analysis of individual maser source using X-ray penetrability to explore maser host obscured AGN; multi-wavelength statistical properties of the whole published H$_{2}$O maser sample. Here their nuclear radio properties were investigated in detail, based on their 6-cm and 20-cm radio observation data. Comparing the radio properties between maser-detected sources and non-detected sources at similar distance scale, we find that: (1) maser host galaxies tend to have higher nuclear radio luminosity; (2) the spectral index of both samples is comparable (∼0.6), within the error ranges. In addition, for AGN-maser sources, the isotropic maser luminosity tends to increase with rising radio luminosity. Thus we propose the nuclear radio luminosity as one good indicator for searching AGN-masers in the future. |
| Starting Page | 37 |
| Ending Page | 41 |
| Page Count | 5 |
| File Format | |
| ISSN | 02506335 |
| Journal | Journal of Astrophysics and Astronomy |
| Volume Number | 32 |
| Issue Number | 1-2 |
| e-ISSN | 09737758 |
| Language | English |
| Publisher | Springer-Verlag |
| Publisher Date | 2011-07-30 |
| Publisher Institution | Indian Academy of Sciences |
| Publisher Place | India |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Maser multi-wavelengt statistics AGN Astrophysics and Astroparticles Astronomy, Observations and Techniques |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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