Abstract
The results of magnesium-to-iron ratio estimates are presented for the nuclei and central bulges of disk galaxies. A great variety of behaviours is found: the nuclei have solar Mg/Fe ratio or are Mg-overabundant, the bulges can be more or less Mg-overabundant than the nuclei. But the most bulges have nearly solar Mg/Fe ratios, irrespective of their luminosity.
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.
