The halo of M 105 and its group environment as traced by planetary nebula populations II. Using kinematics of single stars to unveil the presence of intragroup light around the Leo I galaxies NGC 3384 and M 105 (2022)
Attributed to:
Astrophysics at the University of Nottingham 2020-2023
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202243117
Publication URI: http://dx.doi.org/10.1051/0004-6361/202243117
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics