MUSE observations of dwarf galaxies and a stellar stream in the M 83 group

Spectroscopy for faint dwarf galaxies outside of our own Local Group is challenging. Here, we present MUSE spectroscopy to study the properties of four known dwarf satellites and one stellar stream (KK 208) surrounding the nearby grand spiral M 83, which resides together with the lenticular galaxy Cen A in the Centaurus group. This data completes the phase-space information for all known dwarf galaxies around M 83 down to a completeness of −10 mag in the V band. All studied objects have an intermediate to old and metal-poor stellar population and follow the stellar luminosity-metallicity relation defined by the Local Group dwarfs. For the stellar stream, we serendipitously identify a previously unknown globular cluster that is old and metal-poor. Two dwarf galaxies (NGC 5264 and dw1341-29) may be a bound satellite of a satellite system due to their proximity and shared velocities. With our access to the positions and velocities of 13 dwarfs around M 83, we estimated the mass of the group with different estimators. Ranging between 1.3 and 3.0 × 10 12 M ⊙ for the halo mass, we find it to be larger than previously assumed. This may impact the previously reported tension for cold dark matter cosmology with the count of dwarf galaxies. In contrast to Cen A, we do not find a corotating plane of satellites around M 83.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-05-28
DOI
https://doi.org/10.1051/0004-6361/202452923
Citations
3
Primary Topic
Astronomy and Astrophysical Research
Type
article
Field-Weighted Citation Impact
3.58

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article

MUSE observations of dwarf galaxies and a stellar stream in the M 83 group

Marcel S. Pawlowski, M. Rejkuba, Salvatore Taibi, Oliver Müller et al.
3 citations
Astronomy and Astrophysics
Astronomy and Astrophysical Research
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article

MUSE observations of dwarf galaxies and a stellar stream in the M 83 group

Marcel S. Pawlowski, M. Rejkuba, Salvatore Taibi, Oliver Müller, Katja Fahrion, Noam I. Libeskind, M. Hilker, Federico Lelli, Nick Heesters, Benoît Famaey, Sarah Pearson
article en
3 citations

Abstract

Spectroscopy for faint dwarf galaxies outside of our own Local Group is challenging. Here, we present MUSE spectroscopy to study the properties of four known dwarf satellites and one stellar stream (KK 208) surrounding the nearby grand spiral M 83, which resides together with the lenticular galaxy Cen A in the Centaurus group. This data completes the phase-space information for all known dwarf galaxies around M 83 down to a completeness of −10 mag in the V band. All studied objects have an intermediate to old and metal-poor stellar population and follow the stellar luminosity-metallicity relation defined by the Local Group dwarfs. For the stellar stream, we serendipitously identify a previously unknown globular cluster that is old and metal-poor. Two dwarf galaxies (NGC 5264 and dw1341-29) may be a bound satellite of a satellite system due to their proximity and shared velocities. With our access to the positions and velocities of 13 dwarfs around M 83, we estimated the mass of the group with different estimators. Ranging between 1.3 and 3.0 × 10 12 M ⊙ for the halo mass, we find it to be larger than previously assumed. This may impact the previously reported tension for cold dark matter cosmology with the count of dwarf galaxies. In contrast to Cen A, we do not find a corotating plane of satellites around M 83.

Astronomy and AstrophysicsVol. 699
University of Copenhagen (DK), Centre National de la Recherche Scientifique (FR), University of Vienna (AT), European Southern Observatory (DE), University of Cambridge (GB), Leibniz Institute for Astrophysics Potsdam (DE), Arcetri Astrophysical Observatory (IT), Observatoire astronomique de Strasbourg (FR), European Space Research and Technology Centre (NL), École Polytechnique Fédérale de Lausanne (CH), Université de Strasbourg (FR)
National Science Foundation, Villum Fonden, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, HORIZON EUROPE Framework Programme, Leibniz-Gemeinschaft, HORIZON EUROPE Marie Sklodowska-Curie Actions
Openalex Percentile: Top 8%
Astronomy and Astrophysical Research
3.58
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