A deep photographic image of M83 taken using the UK Schmidt Telescope by Malin & Hadley (1997, figure reproduced with permission) where the white scale bar corresponds to 30 arcmin. The northern stream appears not to be associated with dw1335-29, circled in red. Credit: Carrillo et al., 2016. (Phys.org)—Astronomers have found a new dwarf satellite of Messier 83 (M83, also known as the Southern Pinwheel Galaxy) located some 85,000 light years from its host. This satellite galaxy was designated dw1335-29 and could be an irregular or a transition dwarf. The findings were presented in a paper published Nov. 30 on arXiv.org. Messier 83 is one of the closest and brightest barred spiral galaxies. It is located about 15 million light years away in the constellation Hydra. Finding new satellites of galaxies beyond the Local Group such as Messier 83 could provide essential insights on galaxy formation in a cosmological context.
In 2015, the detection of 16 dwarf galaxy candidates near Messier 83 was announced. However, it remained unclear which of them were satellites of this galaxy. To confirm this, follow-up observations were needed to estimate reliable distances.
Now, a team of astronomers led by Andreia Carrillo of the University of Michigan used images from the Galaxy Halos, Outer disks, Substructure, Thick disks and Star clusters (GHOSTS) survey provided by the Hubble Space Telescope (HST) and data from the Very Large Telescope’s (VLT) Visible MultiObject Spectrograph (VIMOS) to confirm that one of the 16 candidates is indeed a satellite of Messier 83.
”Using a combination of VIMOS ground-based data and HST resolved stellar imaging, we have confirmed that the dwarf candidate dw1335-29 is indeed a satellite of M83,” the researchers wrote in the paper.
The team explained that they detected an overdensity of primarily red giant branch-colored stars with a modest overdensity of blue stars at the position of dw1335-29, confirming it to be a nearby dwarf galaxy. Moreover, it permitted them to estimate its distance from Messier 83 and allowed surface brightness profile measurements.
According to the research, dw1335-29 has a half light radius of approximately 2,140 light years and an ellipticity of 0.4. The scientists found that this dwarf is dominated by an old metal-poor stellar population and its metallicity [Fe/H] is -1.3. The team also noted that it is the faintest confirmed member of the Messier 83 group.
Finally, dw1335-29 has been classified as a dwarf irregular or transition dwarf due to its irregular shape and the likely presence of a star-forming region.
”Owing to dw1335-29’s somewhat irregular shape and possible young stars, we classify this galaxy as a dwarf irregular or transition dwarf. This is curious, as with a projected distance of 26 kpc from M83, dw1335-29 is expected to lack recent star formation,” the paper reads.
The researchers assume that perhaps dw1335-29 has a larger M83-centric distance and is coincidentally projected close to its host, or perhaps the galaxy lacks a sufficiently dense hot gas envelope to quench star formation in its satellites. They hope that a comprehensive census of Messier 83 satellites and their star formation properties would help to resolve this issue.
”Further study of M83’s dwarf population will reveal if star formation in its satellites is commonplace (suggesting a lack of a hot gas envelope for M83 that would quench star formation) or rare (suggesting that dw1335-29 has a larger M83-centric distance, and is fortuitously projected to small radii),” the team concluded.
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More information: Characterizing dw1335-29, a recently discovered dwarf satellite of M83, arXiv:1611.10361 [astro-ph.GA] arxiv.org/abs/1611.10361
The number, distribution, and properties of dwarf satellites are crucial probes of the physics of galaxy formation at low masses and the response of satellite galaxies to the tidal and gas dynamical effects of their more massive parent.To make progress, it is necessary to augment and solidify the census of dwarf satellites of galaxies outside the Local Group. M”uller et al. (2015) presented 16 dwarf galaxy candidates near M83, but lacking reliable distances, it is unclear which candidates are M83 satellites. Using red giant branch stars from the HST/GHOSTS survey in conjunction with ground-based images from VLT/VIMOS, we confirm that one of the candidates, dw1335-29— with a projected distance of 26 kpc from M83 and a distance modulus of (m−M)0=28.5+0.3−0.1—is a satellite of M83. We estimate an absolute magnitude MV=−10.1±0.4, an ellipticity of 0.40+0.14−0.22, a half light radius of 656+121−170 pc, and [Fe/H] = −1.3+0.3−0.4. Owing to dw1335-29’s somewhat irregular shape and possible young stars, we classify this galaxy as a dwarf irregular or transition dwarf. This is curious, as with a projected distance of 26 kpc from M83, dw1335-29 is expected to lack recent star formation. Further study of M83’s dwarf population will reveal if star formation in its satellites is commonplace (suggesting a lack of a hot gas envelope for M83 that would quench star formation) or rare (suggesting that dw1335-29 has a larger M83-centric distance, and is fortuitously projected to small radii).
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