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

Hartke, J.; Arnaboldi, M.; Gerhard, O.; Coccato, L.; Merrifield, M.; Kuijken, K.H.; Pulsoni, C.; Agnello, A.; Bhattacharya, S.; Spiniello, C.; Cortesi, A.; Freeman, K.C.; Napolitano, N.R.; Romanowsky, A.J.

doi:10.1051/0004-6361/202243117

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

Author(s):: Hartke, J.; Arnaboldi, M.; Gerhard, O.; Coccato, L.; Merrifield, M.; Kuijken, K.H. (0000-0002-3827-0175); Pulsoni, C.; Agnello, A.; Bhattacharya, S.; Spiniello, C.; Cortesi, A.; Freeman, K.C.; Napolitano, N.R.; Romanowsky, A.J.

Published: 2022
Publication type: Article / Letter to editor

Galaxies - individual - M 105Galaxies - elliptical and lenticular cDGalaxies - groups - individual - Leo IGalaxies - halosPlanetary nebulae - generalAstrophysics - astrophysics of galaxies

Date issued: 2022
Language: English
Is part of: Astronomy & Astrophysics (2022), A12
hdl: 1887/3514471
doi: 10.1051/0004-6361/202243117
URL: https://ui.adsabs.harvard.edu/abs/2022A&A...663A..12H

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

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