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arXiv · 2503.03242

Chemical signature reveals co-spatial dwarf satellite of an edge-on disc galaxy with MUSE

Devang Somawanshi·Souradeep Bhattacharya·Manish Kataria·Preetish K. Mishra·Chiaki Kobayashi
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Abstract

Integral field unit (IFU) spectroscopic observations of resolved galaxies provide an optimal experimental setting for determination of stellar population properties, in particular - age, metallicity and $α$-enhancement, which are key to understanding evolution of galaxies across diverse physical environments. We determine these properties for the edge-on disc galaxy IC 1553, through stellar population models fitted to MUSE IFU observations. From our determined spatial distributions of metallicity and [$α$/Fe], we serendipitiously identify the unique chemical signature of a dwarf galaxy that is co-spatial with the luminous disc of IC 1553. The dwarf galaxy is characterized by the presence of higher [$α$/Fe] and metal-poor stellar populations relative to the disc of IC 1553. The identified dwarf is dynamically cold from its determined kinematics, consistent with being a satellite of IC 1553. From modeling the Spitzer IRAC 3.6 $μm$ image of IC 1553, we confirmed the presence of the dwarf galaxy and calculated its stellar mass to be $\sim1.28\times 10^{9} \rm~M_{\odot}$. This is the first such identification of a dwarf galaxy from its unique chemical signature in such integrated light IFU observations, even though its hidden by the luminous body of its massive host.

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Devang Somawanshi, Souradeep Bhattacharya, Manish Kataria, Preetish K. Mishra, Chiaki Kobayashi. 2025-05-11. Chemical signature reveals co-spatial dwarf satellite of an edge-on disc galaxy with MUSE. https://arxiv.org/abs/2503.03242

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