4.7 Article

The Streams of the Gaping Abyss: A Population of Entangled Stellar Streams Surrounding the Inner Galaxy

Journal

ASTROPHYSICAL JOURNAL
Volume 872, Issue 2, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/ab0080

Keywords

galaxies: formation; Galaxy: halo; Galaxy: stellar content; Galaxy: structure; surveys

Funding

  1. Alfred P. Sloan Foundation
  2. National Science Foundation
  3. U.S. Department of Energy Office of Science
  4. University of Arizona
  5. Brazilian Participation Group
  6. Brookhaven National Laboratory
  7. Carnegie Mellon University
  8. University of Florida
  9. French Participation Group
  10. German Participation Group
  11. Harvard University
  12. Instituto de Astrofisica de Canarias
  13. Michigan State/Notre Dame/JINA Participation Group
  14. Johns Hopkins University
  15. Lawrence Berkeley National Laboratory
  16. Max Planck Institute for Astrophysics
  17. Max Planck Institute for Extraterrestrial Physics
  18. New Mexico State University
  19. New York University
  20. Ohio State University
  21. Pennsylvania State University
  22. University of Portsmouth
  23. Princeton University
  24. Spanish Participation Group
  25. University of Tokyo
  26. University of Utah
  27. Vanderbilt University
  28. University of Virginia
  29. University of Washington
  30. Yale University
  31. National Development and Reform Commission
  32. French National Research Agency
  33. Programme National Cosmologie et Galaxies grant

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We present the discovery of a large population of stellar streams that surround the inner Galaxy, found in the Gaia DR2 catalog using the new STREAMFINDER algorithm. Here we focus on the properties of eight new high-significance structures found at heliocentric distances between 1 and 10 kpc and at Galactic latitudes vertical bar b vertical bar > 20 degrees, named Slidr, Sylgr, Ylgr, Fimbulthul, Svol, Fjorm, Gjoll, and Leiptr. Spectroscopic measurements of seven of the streams confirm the detections, which are based on Gaia astrometry and photometry alone, and show that these streams are predominantly metal-poor. The sample possesses diverse orbital properties, although most of the streams appear to be debris of inner-halo globular clusters. Many more candidate streams are visible in our maps but require follow-up spectroscopy to confirm their nature. We also explain in detail the workings of the algorithm and gauge the incidence of false detections by running the algorithm on a smooth model of the Gaia catalog.

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