The role of AGN and its obscuration on the position of the host galaxy relative to Main Sequence
2021
We use X-ray Active Galactic Nuclei (AGN) observed by the Chandra X-ray Observatory within the 9.3 deg$^2$ Bo$\rm \ddot{o}$tes field of the NDWFS to study whether there is a correlation between X-ray luminosity (L$_X$) and star formation rate (SFR) of the host galaxy, at $\rm 0.5
Keywords:
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
110
References
0
Citations
NaN
KQI