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Hauptverfasser: Jiménez-Teja, Yolanda, Román, Javier, HyeongHan, Kim, Vílchez, Jose M., Dupke, Renato A., Lopes, Paulo Afrânio Augusto, Rich, Robert Michael, Caceres, Osmin, Li, Chester
Format: Preprint
Veröffentlicht: 2024
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Online-Zugang:https://arxiv.org/abs/2412.15328
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author Jiménez-Teja, Yolanda
Román, Javier
HyeongHan, Kim
Vílchez, Jose M.
Dupke, Renato A.
Lopes, Paulo Afrânio Augusto
Rich, Robert Michael
Caceres, Osmin
Li, Chester
author_facet Jiménez-Teja, Yolanda
Román, Javier
HyeongHan, Kim
Vílchez, Jose M.
Dupke, Renato A.
Lopes, Paulo Afrânio Augusto
Rich, Robert Michael
Caceres, Osmin
Li, Chester
contents Detection and study of the intracluster light in rich clusters of galaxies has been a problem of long standing challenge and interest. Using the lowest surface brightness images of the Coma cluster of galaxies in the g and r bands, from the Halos and Environment of Nearby Galaxies (HERON) Coma Cluster Project, we obtained the most extensive image of intracluster light (ICL) in a single cluster to date, spreading over 1.5 Mpc from the cluster core. The unprecedented wealth of spectroscopic data made publicly available by the Dark Energy Spectroscopic Instrument (DESI) Early Data Release, complemented with a compilation from the NASA/IPAC Extragalactic Database and the literature, enabled the identification of 2,157 galaxy members within Coma, from which 42 distinct groups were identified. The synergy between these high-quality data allowed us to: 1) calculate ICL fractions of $19.9\pm0.5$\% and $19.6\pm0.6$\% in the g and r bands, respectively, consistent with a dynamically active cluster, 2) unveil Coma's faintest tidal features, and 3) provide a comprehensive picture of the dynamics and interactions within this complex system. Our findings indicate that the ICL connects several of these groups in a filamentous network, from which we infer the ongoing dynamical processes. In particular, we identified a faint stellar bridge linking the core of Coma with the galaxy NGC 4839, providing compelling evidence that this galaxy has already traversed the central region of the cluster.
format Preprint
id arxiv_https___arxiv_org_abs_2412_15328
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Deep view of the intracluster light in the Coma cluster of galaxies
Jiménez-Teja, Yolanda
Román, Javier
HyeongHan, Kim
Vílchez, Jose M.
Dupke, Renato A.
Lopes, Paulo Afrânio Augusto
Rich, Robert Michael
Caceres, Osmin
Li, Chester
Astrophysics of Galaxies
Detection and study of the intracluster light in rich clusters of galaxies has been a problem of long standing challenge and interest. Using the lowest surface brightness images of the Coma cluster of galaxies in the g and r bands, from the Halos and Environment of Nearby Galaxies (HERON) Coma Cluster Project, we obtained the most extensive image of intracluster light (ICL) in a single cluster to date, spreading over 1.5 Mpc from the cluster core. The unprecedented wealth of spectroscopic data made publicly available by the Dark Energy Spectroscopic Instrument (DESI) Early Data Release, complemented with a compilation from the NASA/IPAC Extragalactic Database and the literature, enabled the identification of 2,157 galaxy members within Coma, from which 42 distinct groups were identified. The synergy between these high-quality data allowed us to: 1) calculate ICL fractions of $19.9\pm0.5$\% and $19.6\pm0.6$\% in the g and r bands, respectively, consistent with a dynamically active cluster, 2) unveil Coma's faintest tidal features, and 3) provide a comprehensive picture of the dynamics and interactions within this complex system. Our findings indicate that the ICL connects several of these groups in a filamentous network, from which we infer the ongoing dynamical processes. In particular, we identified a faint stellar bridge linking the core of Coma with the galaxy NGC 4839, providing compelling evidence that this galaxy has already traversed the central region of the cluster.
title Deep view of the intracluster light in the Coma cluster of galaxies
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2412.15328