The DOI matches its Crossref record; 61 of the 61 references it cites were found in a registry or an index.
Evidence for Stellar Substructure in the Halo and Outer Disk of M31
Open accessAbstract
We report the discovery of significant stellar substructure in the halo and outer disk of our nearest large galactic neighbor, M31. Our deep panoramic survey with the Isaac Newton Telescope Wide Field Camera currently maps out an area of ≈25 deg 2 around M31, extending along the semimajor axis to 55 kpc and is the first to allow an uninterrupted study of the density and color distribution of individual red giant branch stars across a large fraction of the halo of an external spiral galaxy. We find evidence for both spatial density and metallicity (as inferred from color information) variations, which are often, but not always, correlated. In addition to the previously reported giant stellar stream, the data reveal the presence of significant stellar overdensities at large radii close to the southwestern major axis, in the proximity of the very luminous globular cluster G1, and near the northeastern major axis, coinciding with and extending beyond the previously known northern spur. The most prominent metallicity variations are found in the southern half of the halo, where two large structures with above average metallicites are apparent; one of these coincides with the giant stellar stream while the other corresponds to a much lower level stellar enhancement. Our findings contrast with, but do not conflict with, past studies of the M31 halo and outer disk that have suggested a rather homogeneous stellar population at large radius: the bulk of our newly detected substructure lies in the previously uncharted far outer regions of the galaxy. We discuss the possible origin of the substructure observed and the implications it has for constraining the galaxy assembly process.
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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
Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
White, S. D. M., & Rees, M. J. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/183.3.341 · Cited by 3,919
Dark Matter Substructure within Galactic Halos
Moore, B., Ghigna, S., Governato, F., Lake, G., Quinn, T., Stadel, J., & Tozzi, P. (1999) · The Astrophysical Journal · doi:10.1086/312287 · Cited by 3,021
Where Are the Missing Galactic Satellites?
Klypin, A., Kravtsov, A. V., Valenzuela, O., & Prada, F. (1999) · The Astrophysical Journal · doi:10.1086/307643 · Cited by 2,741
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. (2000) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:2000126 · Cited by 2,553
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
The origin of dwarf galaxies, cold dark matter, and biased galaxy formation
Dekel, A., & Silk, J. (1986) · The Astrophysical Journal · doi:10.1086/164050 · Cited by 1,919 · cited 1×
“…stellar component, either due to feedback from early star formation, that expels the gas before significant star formation can occur (e.g., White & Rees 1978; Dekel & Silk 1986), or from the inhibition of gas cooling due to an ionizing UV background (e.g., Bullock, Kravtsov, & Weinberg 2000).”
BackgroundReionization and the Abundance of Galactic Satellites
Bullock, J. S., Kravtsov, A. V., & Weinberg, D. H. (2000) · The Astrophysical Journal · doi:10.1086/309279 · Cited by 877
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-citationStructural parameters for the Galactic dwarf spheroidals
Irwin, M., & Hatzidimitriou, D. (1995) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/277.4.1354 · Cited by 602
Self-citation
Cited by
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
The remnants of galaxy formation from a panoramic survey of the region around M31
McConnachie, A. W., Irwin, M. J., Ibata, R. A., Dubinski, J., Widrow, L. M., Martin, N. F., Côté, P., Dotter, A. L., Navarro, J. F., Ferguson, A. M. N., et al. (2009) · Nature · doi:10.1038/nature08327 · Cited by 621
Self-citationGalactic 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
Distances and metallicities for 17 Local Group galaxies
McConnachie, A. W., Irwin, M. J., Ferguson, A. M. N., Ibata, R. A., Lewis, G. F., & Tanvir, N. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08514.x · Cited by 533
Self-citationThe Accretion Origin of the Milky Way’s Stellar Halo
Bell, E. F., Zucker, D. B., Belokurov, V., Sharma, S., Johnston, K. V., Bullock, J. S., Hogg, D. W., Jahnke, K., de Jong, J. T. A., Beers, T. C., et al. (2008) · The Astrophysical Journal · doi:10.1086/588032 · Cited by 444
Metadata
- Authors
- Ferguson, A. M. N., Irwin, M. J., Ibata, R. A., Lewis, G. F., & Tanvir, N. R.
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2002-09
- Volume
- 124
- Issue
- 3
- Pages
- 1452-1463
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2130764799
- Cited by
- 416
- References
- 61
- FWCI
- 19.89
- Type
- journal article
- Language
- en
- Open access
- bronze
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