Is Ursa Major II the progenitor of the Orphan Stream?

M. Fellhauer, N. W. Evans, V. Belokurov, D. B. Zucker, B. Yanny, M. I. Wilkinson, G. Gilmore, M. J. Irwin, D. M. Bramich, S. Vidrih, P. Hewett, T. Beers

Research output: Contribution to journalArticle

45 Citations (Scopus)

Abstract

Prominent in the 'Field of Streams' - the Sloan Digital Sky Survey map of substructure in the Galactic halo - is an 'Orphan Stream' without obvious progenitor. In this numerical study, we show a possible connection between the newly found dwarf satellite Ursa Major II (UMa II) and the Orphan Stream. We provide numerical simulations of the disruption of UMa II that match the observational data on the position, distance and morphology of the Orphan Stream. We predict the radial velocity of UMa II as - 100 km s-1, as well as the existence of strong velocity gradients along the Orphan Stream. The velocity dispersion of UMa II is expected to be high, though this can be caused both by a high dark matter content or by the presence of unbound stars in a disrupted remnant. However, the existence of a gradient in the mean radial velocity across UMa II provides a clear-cut distinction between these possibilities. The simulations support the idea that some of the anomalous, young halo globular clusters like Palomar 1 or Arp 2 or Ruprecht 106 may be physically associated with the Orphan Stream.

Original languageEnglish
Pages (from-to)1171-1179
Number of pages9
JournalMonthly Notices of the Royal Astronomical Society
Volume375
Issue number4
DOIs
Publication statusPublished - 1 Mar 2007
Externally publishedYes

Fingerprint

orphan
radial velocity
gradients
galactic halos
globular clusters
substructures
simulation
halos
dark matter
stars

Keywords

  • Galaxies: dwarf
  • Galaxies: evolution
  • Galaxies: individual: UMa II
  • Galaxies: kinematics and dynamics
  • Methods: N-body simulations

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Fellhauer, M., Evans, N. W., Belokurov, V., Zucker, D. B., Yanny, B., Wilkinson, M. I., ... Beers, T. (2007). Is Ursa Major II the progenitor of the Orphan Stream? Monthly Notices of the Royal Astronomical Society, 375(4), 1171-1179. https://doi.org/10.1111/j.1365-2966.2006.11404.x

Is Ursa Major II the progenitor of the Orphan Stream? / Fellhauer, M.; Evans, N. W.; Belokurov, V.; Zucker, D. B.; Yanny, B.; Wilkinson, M. I.; Gilmore, G.; Irwin, M. J.; Bramich, D. M.; Vidrih, S.; Hewett, P.; Beers, T.

In: Monthly Notices of the Royal Astronomical Society, Vol. 375, No. 4, 01.03.2007, p. 1171-1179.

Research output: Contribution to journalArticle

Fellhauer, M, Evans, NW, Belokurov, V, Zucker, DB, Yanny, B, Wilkinson, MI, Gilmore, G, Irwin, MJ, Bramich, DM, Vidrih, S, Hewett, P & Beers, T 2007, 'Is Ursa Major II the progenitor of the Orphan Stream?', Monthly Notices of the Royal Astronomical Society, vol. 375, no. 4, pp. 1171-1179. https://doi.org/10.1111/j.1365-2966.2006.11404.x
Fellhauer M, Evans NW, Belokurov V, Zucker DB, Yanny B, Wilkinson MI et al. Is Ursa Major II the progenitor of the Orphan Stream? Monthly Notices of the Royal Astronomical Society. 2007 Mar 1;375(4):1171-1179. https://doi.org/10.1111/j.1365-2966.2006.11404.x
Fellhauer, M. ; Evans, N. W. ; Belokurov, V. ; Zucker, D. B. ; Yanny, B. ; Wilkinson, M. I. ; Gilmore, G. ; Irwin, M. J. ; Bramich, D. M. ; Vidrih, S. ; Hewett, P. ; Beers, T. / Is Ursa Major II the progenitor of the Orphan Stream?. In: Monthly Notices of the Royal Astronomical Society. 2007 ; Vol. 375, No. 4. pp. 1171-1179.
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