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Cited by 418

The DOI matches its Crossref record; 10 of the 10 references it cites were found in a registry or an index.

A Low‐Latitude Halo Stream around the Milky Way

Open access
Yanny, Brian, Newberg, Heidi Jo, Grebel, Eva K., Kent, Steve, Odenkirchen, Michael, Rockosi, Connie M., Schlegel, David, Subbarao, Mark, Brinkmann, Jon, Fukugita, Masataka, Ivezic, Željko, Lamb, Don Q., Schneider, Donald P., York, Donald G.·2003·The Astrophysical Journal

Abstract

We present evidence for a ring of stars in the plane of the Milky Way, extending at least from l = 180° to 227° with turnoff magnitude g ~ 19.5; the ring could encircle the Galaxy. We infer that the low Galactic latitude structure is at a fairly constant distance of R = 18 ± 2 kpc from the Galactic center above the Galactic plane and has R = 20 ± 2 kpc in the region sampled below the Galactic plane. The evidence includes 500 Sloan Digital Sky Survey spectroscopic radial velocities of stars within 30° of the plane. The velocity dispersion of the stars associated with this structure is found to be 27 km s -1 at ( l , b ) = (198°, - 27°), 22 km s -1 at ( l , b ) = (225°, 28°), 30 km s -1 at ( l , b ) = (188°, 24°), and 30 km s -1 at ( l , b ) = (182°, 27°). The structure rotates in the same prograde direction as the Galactic disk stars but with a circular velocity of 110 ± 25 km s -1 . The narrow measured velocity dispersion is inconsistent with power-law spheroid or thick-disk populations. We compare the velocity dispersion in this structure with the velocity dispersion of stars in the Sagittarius dwarf galaxy tidal stream, for which we measure a velocity dispersion of 20 km s -1 at ( l , b ) = (165°, - 55°). We estimate a preliminary metallicity from the Ca II (K) line and color of the turnoff stars of [Fe/H] = -1.6 with a dispersion of 0.3 dex and note that the turnoff color is consistent with that of the spheroid population. We interpret our measurements as evidence for a tidally disrupted satellite of 2 × 10 7 to 5 × 10 8 M ☉ that rings the Galaxy.

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Metadata

Authors
Yanny, B., Newberg, H. J., Grebel, E. K., Kent, S., Odenkirchen, M., Rockosi, C. M., Schlegel, D., Subbarao, M., Brinkmann, J., Fukugita, M., Ivezic, Ž., Lamb, D. Q., Schneider, D. P., & York, D. G.
Venue
The Astrophysical Journal
Published
2003-05-10
Volume
588
Issue
2
Pages
824-841
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2025254193
Cited by
418
References
10
FWCI
24.94
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: A Low‐Latitude Halo Stream around the Milky Way. https://app.cochat.ai/papers/10.1086/374220
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Yanny, B., Newberg, H. J., Grebel, E. K., Kent, S., Odenkirchen, M., Rockosi, C. M., Schlegel, D., Subbarao, M., Brinkmann, J., Fukugita, M., Ivezic, Ž., Lamb, D. Q., Schneider, D. P., & York, D. G. (2003). A Low‐Latitude Halo Stream around the Milky Way. The Astrophysical Journal. https://doi.org/10.1086/374220

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