Evidence for Ultra-diffuse Galaxy Formation through Tidal Heating of Normal Dwarfs

Michael G. Jones, Paul Bennet, Burcin Mutlu-Pakdil, David J. Sand, Kristine Spekkens, Denija Crnojević, Ananthan Karunakaran, Dennis Zaritsky

Research output: Contribution to journalArticlepeer-review

Abstract

We have followed up two ultra-diffuse galaxies (UDGs), detected adjacent to stellar streams, with Hubble Space Telescope (HST) imaging and H i mapping with the Jansky Very Large Array in order to investigate the possibility that they might have a tidal origin. With the HST F814W and F555W images we measure the globular cluster (GC) counts for NGC 2708-Dw1 and NGC 5631-Dw1 as 2-1+1 and 5-2+1, respectively. NGC 2708-Dw1 is undetected in H i down to a 3σ limit of log (M H i /M o˙) = 7.3, and there is no apparent H i associated with the nearby stellar stream. There is a 2σ H i feature coincident with NGC 5631-Dw1. However, this emission is blended with a large gaseous tail emanating from NGC 5631 and is not necessarily associated with the UDG. The presence of any GCs and the lack of clear H i connections between the UDGs and their parent galaxies strongly disfavor a tidal dwarf galaxy origin, but cannot entirely rule it out. The GC counts are consistent with those of normal dwarf galaxies, and the most probable formation mechanism is one where these UDGs were born as normal dwarfs and were later tidally stripped and heated. We also identify an overluminous (M V = -11.1) GC candidate in NGC 2708-Dw1, which may be a nuclear star cluster transitioning to an ultra-compact dwarf as the surrounding dwarf galaxy gets stripped of stars.

Original languageEnglish (US)
Article number72
JournalAstrophysical Journal
Volume919
Issue number2
DOIs
StatePublished - Oct 1 2021

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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