Abstract
ABSTRACT A compilation was made of the total number of globular clusters associated with M 104, M87, and all the members of the Local Croup except for the Magellanic Clouds. We found that the total number of clusters in a galaxy increases approximately linearly as the luminosity of the spheroidal system of a parent galaxy increases, where the spheroidal system means the spheroidal central bulge for the spiral galaxies, or the whole system for elliptical galaxies. Key words: globular clusters-spheroidal central bulge-galaxies
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 callMore From: Publications of the Astronomical Society of the Pacific
Disclaimer: 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.
