Pavel E. Mancera Piña
Off the Baryonic Tully–Fisher Relation: A Population of Baryon-dominated Ultra-diffuse Galaxies
Mancera Piña, Pavel E.; Fraternali, Filippo; Adams, Elizabeth A.K.; Marasco, Antonino; Oosterloo, Tom; Oman, Kyle A.; Leisman, Lukas; di Teodoro, Enrico M.; Posti, Lorenzo; Battipaglia, Michael; Cannon, John M.; Gault, Lexi; Haynes, Martha P.; Janowiecki, Steven; McAllan, Elizabeth; Pagel, Hannah J.; Reiter, Kameron; Rhode, Katherine L.; Salzer, John J.; Smith, Nicholas J.
Authors
Filippo Fraternali
Elizabeth A.K. Adams
Antonino Marasco
Tom Oosterloo
Dr Kyle Oman kyle.a.oman@durham.ac.uk
Associate Professor - Royal Society Dorothy Hodgkin Fellow
Lukas Leisman
Enrico M. di Teodoro
Lorenzo Posti
Michael Battipaglia
John M. Cannon
Lexi Gault
Martha P. Haynes
Steven Janowiecki
Elizabeth McAllan
Hannah J. Pagel
Kameron Reiter
Katherine L. Rhode
John J. Salzer
Nicholas J. Smith
Abstract
We study the gas kinematics traced by the 21 cm emission of a sample of six H i-rich low surface brightness galaxies classified as ultra-diffuse galaxies (UDGs). Using the 3D kinematic modeling code 3DBarolo we derive robust circular velocities, revealing a startling feature: H i-rich UDGs are clear outliers from the baryonic Tully–Fisher relation, with circular velocities much lower than galaxies with similar baryonic mass. Notably, the baryon fraction of our UDG sample is consistent with the cosmological value: these UDGs are compatible with having no "missing baryons" within their virial radii. Moreover, the gravitational potential provided by the baryons is sufficient to account for the amplitude of the rotation curve out to the outermost measured point, contrary to other galaxies with similar circular velocities. We speculate that any formation scenario for these objects will require very inefficient feedback and a broad diversity in their inner dark matter content.
Citation
Mancera Piña, P. E., Fraternali, F., Adams, E. A., Marasco, A., Oosterloo, T., Oman, K. A., Leisman, L., di Teodoro, E. M., Posti, L., Battipaglia, M., Cannon, J. M., Gault, L., Haynes, M. P., Janowiecki, S., McAllan, E., Pagel, H. J., Reiter, K., Rhode, K. L., Salzer, J. J., & Smith, N. J. (2019). Off the Baryonic Tully–Fisher Relation: A Population of Baryon-dominated Ultra-diffuse Galaxies. Astrophysical Journal Letters, 883(2), Article L33. https://doi.org/10.3847/2041-8213/ab40c7
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 1, 2019 |
Online Publication Date | Sep 25, 2019 |
Publication Date | Oct 1, 2019 |
Deposit Date | Oct 27, 2021 |
Publicly Available Date | Oct 27, 2021 |
Journal | Astrophysical Journal Letters |
Print ISSN | 2041-8205 |
Electronic ISSN | 2041-8213 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 883 |
Issue | 2 |
Article Number | L33 |
DOI | https://doi.org/10.3847/2041-8213/ab40c7 |
Public URL | https://durham-repository.worktribe.com/output/1224988 |
Related Public URLs | https://arxiv.org/pdf/1909.01363 |
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Copyright Statement
This is an author-created, un-copyedited version of an article published in Astrophysical Journal Letters. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version
derived from it. The Version of Record is available online at https://doi.org/10.3847/2041-8213/ab40c7
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