📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

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)

First Author: Hartke J

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