The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.
One ring to encompass them all: a giant stellar structure that surrounds the Galaxy
Open accessAbstract
We present evidence that the curious stellar population found by the Sloan Digital Sky Survey in the Galactic anticentre direction extends to other distant fields that skirt the plane of the Milky Way.New data, taken with the Isaac Newton Telescope Wide Field Camera, show a similar population, narrowly aligned along the line of sight, but with a galactocentric distance that changes from ∼15 to ∼20 kpc (over ∼100° on the sky).Despite being narrowly concentrated along the line of sight, the structure is fairly extended vertically out of the plane of the disc, with a vertical scaleheight of 0.75 ± 0.04 kpc.This finding suggests that the outer rim of the Galaxy ends in a low surface brightness stellar ring.Presently available data do not allow us to ascertain the origin of the structure.One possibility is that it is the wraith of a satellite galaxy devoured long ago by the Milky Way, although our favoured interpretation is that it is a perturbation of the disc, possibly the result of ancient warps.Assuming that the ring is smooth and axisymmetric, the total stellar mass in the structure may amount to ∼2 × 108 M⊙ up to∼109 M⊙.
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Cites
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
Sloan Digital Sky Survey: Early Data Release
Stoughton, C., Lupton, R. H., Bernardi, M., Blanton, M. R., Burles, S., Castander, F. J., Connolly, A. J., Eisenstein, D. J., Frieman, J. A., Hennessy, G. S., et al. (2002) · The Astronomical Journal · doi:10.1086/324741 · Cited by 2,390
DWARF GALAXIES OF THE LOCAL GROUP
Mateo, M. (1998) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.36.1.435 · Cited by 2,362
GAIA: Composition, formation and evolution of the Galaxy
Perryman, M. A. C., de Boer, K. S., Gilmore, G., Høg, E., Lattanzi, M. G., Lindegren, L., Luri, X., Mignard, F., Pace, O., & de Zeeuw, P. T. (2001) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20010085 · Cited by 1,100
Radial mixing in galactic discs
Sellwood, J. A., & Binney, J. J. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2002.05806.x · Cited by 1,054
The Ghost of Sagittarius and Lumps in the Halo of the Milky Way
Newberg, H. J., Yanny, B., Rockosi, C., Grebel, E. K., Rix, H., Brinkmann, J., Csabai, I., Hennessy, G., Hindsley, R. B., Ibata, R., et al. (2002) · The Astrophysical Journal · doi:10.1086/338983 · Cited by 760
Self-citationA giant stream of metal-rich stars in the halo of the galaxy M31
Ibata, R., Irwin, M., Lewis, G., Ferguson, A. M. N., & Tanvir, N. (2001) · Nature · doi:10.1038/35083506 · Cited by 593
Self-citation1 The Ghost of Sagittarius and Lumps in the Halo of the Milky WayPreprint
Newberg, H. J., Yanny, B., Rockosi, C. M., Grebel, E. K., Rix, H. W., Brinkmann, J., Csabai, I., Hennessy, G. S., Hindsley, R. B., Ibata, R., et al. (2001) · Cited by 520
Self-citationThe mass-luminosity relation for stars of mass 1.0 to 0.08 solar mass
Henry, T. J., & McCarthy, D. W., Jr. (1993) · The Astronomical Journal · doi:10.1086/116685 · Cited by 438
The Effects of a Photoionizing Ultraviolet Background on the Formation of Disk Galaxies
Navarro, J. F., & Steinmetz, M. (1997) · The Astrophysical Journal · doi:10.1086/303763 · Cited by 420
Cited by
The Galaxy in Context: Structural, Kinematic, and Integrated Properties
Bland-Hawthorn, J., & Gerhard, O. (2016) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081915-023441 · Cited by 1,656
The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution
Jurić, M., Ivezić, Ž., Brooks, A., Lupton, R. H., Schlegel, D., Finkbeiner, D., Padmanabhan, N., Bond, N., Sesar, B., Rockosi, C. M., et al. (2008) · The Astrophysical Journal · doi:10.1086/523619 · Cited by 1,312
Tracing Galaxy Formation with Stellar Halos. I. Methods
Bullock, J. S., & Johnston, K. V. (2005) · The Astrophysical Journal · doi:10.1086/497422 · Cited by 1,044
Galactic stellar haloes in the CDM model
Cooper, A. P., Cole, S., Frenk, C. S., White, S. D. M., Helly, J., Benson, A. J., De Lucia, G., Helmi, A., Jenkins, A., Navarro, J. F., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16740.x · Cited by 594
THE SAGITTARIUS DWARF GALAXY: A MODEL FOR EVOLUTION IN A TRIAXIAL MILKY WAY HALO
Law, D. R., & Majewski, S. R. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/714/1/229 · Cited by 550
Metadata
- Authors
- Ibata, R. A., Irwin, M. J., Lewis, G. F., Ferguson, A. M. N., & Tanvir, N.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2003-04-11
- Volume
- 340
- Issue
- 3
- Pages
- L21-L27
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2014648872
- Cited by
- 269
- References
- 23
- FWCI
- 17.01
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Ibata, R. A., Irwin, M. J., Lewis, G. F., Ferguson, A. M. N., & Tanvir, N. (2003). One ring to encompass them all: a giant stellar structure that surrounds the Galaxy. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2003.06545.x
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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