Abstract
Our aim is to quantify the stellar population within the nuclear regions of AGN by means of long slit spectroscopic observations in the optical range (5000-10000Å), including MgI, NaI, TiO, CN, CaIIT. We wish to determine whether there is a relationship between central activity and stellar population, and to determine the nature of the featureless continuum.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
