The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
DWARF GALAXIES OF THE LOCAL GROUP
Open accessAbstract
▪ Abstract The Local Group dwarf galaxies offer a unique window to the detailed properties of the most common type of galaxy in the Universe. In this review, I update the census of Local Group dwarfs based on the most recent distance and radial velocity determinations. I then discuss the detailed properties of this sample, including (a) the integrated photometric parameters and optical structures of these galaxies, (b) the content, nature, and distribution of their interstellar medium (ISM), (c) their heavy-element abundances derived from both stars and nebulae, (d) the complex and varied star-formation histories of these dwarfs, (e) their internal kinematics, stressing the relevance of these galaxies to the “dark matter problem” and to alternative interpretations, and (f) evidence for past, ongoing, and future interactions of these dwarfs with other galaxies in the Local Group and beyond. To complement the discussion and to serve as a foundation for future work, I present an extensive set of basic observational data in tables that summarize much of what we know and do not know about these nearby dwarfs. Our understanding of these galaxies has grown impressively in the past decade, but fundamental puzzles remain that will keep the Local Group at the forefront of galaxy evolution studies for some time.
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Citations
Cites
A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis
Milgrom, M. (1983) · The Astrophysical Journal · doi:10.1086/161130 · Cited by 3,316
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×
“Star-formation (Dekel & Silk 1986, Babul & Rees 1992, De Young and Heckman 1994) and ram-pressure stripping (Faber & Lin 1983, van den Bergh 1994c) have been proposed as means of removing gas from dwarfs in the inner Galactic halo.”
Background
Cited by
Particle dark matter: evidence, candidates and constraints
Bertone, G., Hooper, D., & Silk, J. (2005) · Physics Reports · doi:10.1016/j.physrep.2004.08.031 · Cited by 4,979
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
Observational Evidence for Self-Interacting Cold Dark Matter
Spergel, D. N., & Steinhardt, P. J. (2000) · Physical Review Letters · doi:10.1103/physrevlett.84.3760 · Cited by 2,097
Star-Formation Histories, Abundances, and Kinematics of Dwarf Galaxies in the Local Group
Tolstoy, E., Hill, V., & Tosi, M. (2009) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082708-101650 · Cited by 1,179
The New Galaxy: Signatures of Its Formation
Freeman, K., & Bland-Hawthorn, J. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093840 · Cited by 1,160
Metadata
- Authors
- Mateo, M.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 1998-09
- Volume
- 36
- Issue
- 1
- Pages
- 435-506
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2131462302
- Cited by
- 2,362
- References
- 2
- FWCI
- 7.57
- Type
- journal article
- Language
- en
- Open access
- green
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- Mateo, M. (1998). DWARF GALAXIES OF THE LOCAL GROUP. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.36.1.435
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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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