The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
THE UNIVERSAL STELLAR MASS-STELLAR METALLICITY RELATION FOR DWARF GALAXIES
Open accessAbstract
We present spectroscopic metallicities of individual stars in seven gas-rich dwarf irregular galaxies (dIrrs), and we show that dIrrs obey the same mass–metallicity relation as the dwarf spheroidal (dSph) satellites of both the Milky Way and M31: . The uniformity of the relation is in contradiction to previous estimates of metallicity based on photometry. This relationship is roughly continuous with the stellar mass–stellar metallicity relation for galaxies as massive as M * = 10 12 M ☉ . Although the average metallicities of dwarf galaxies depend only on stellar mass, the shapes of their metallicity distributions depend on galaxy type. The metallicity distributions of dIrrs resemble simple, leaky box chemical evolution models, whereas dSphs require an additional parameter, such as gas accretion, to explain the shapes of their metallicity distributions. Furthermore, the metallicity distributions of the more luminous dSphs have sharp, metal-rich cut-offs that are consistent with the sudden truncation of star formation due to ram pressure stripping.
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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
THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
Abazajian, K. N., Adelman-McCarthy, J. K., Agüeros, M. A., Allam, S. S., Prieto, C. A., An, D., Anderson, K. S. J., Anderson, S. F., Annis, J., Bahcall, N. A., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/182/2/543 · Cited by 5,341
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 2×
“The relation can be explained by the retention of metals in the galaxies’ gravitational potential wells (e.g., Dekel & Silk 1986).”
BackgroundTHE OBSERVED PROPERTIES OF DWARF GALAXIES IN AND AROUND THE LOCAL GROUP
McConnachie, A. W. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/144/1/4 · Cited by 1,869
Cited by
The EAGLE project: simulating the evolution and assembly of galaxies and their environments
Schaye, J., Crain, R. A., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2058 · Cited by 3,601
Co-formation of the disc and the stellar halo★
Belokurov, V, Erkal, D., Evans, N. W., Koposov, S. E., & Deason, A. J. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty982 · Cited by 1,020
Evidence for two early accretion events that built the Milky Way stellar halo
Myeong, G. C., Vasiliev, E., Iorio, G., Evans, N. W., & Belokurov, V (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1770 · Cited by 505
Mackereth, J. T., Schiavon, R. P., Pfeffer, J., Hayes, C. R., Bovy, J., Anguiano, B., Prieto, C. A., Hasselquist, S., Holtzman, J., Johnson, J. A., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty2955 · Cited by 285
Reverse engineering the Milky Way
Forbes, D. A. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa245 · Cited by 168
Metadata
- Authors
- Kirby, E. N., Cohen, J. G., Guhathakurta, P., Cheng, L., Bullock, J. S., & Gallazzi, A.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2013-11-27
- Volume
- 779
- Issue
- 2
- Pages
- 102
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2087953910
- Cited by
- 791
- References
- 4
- FWCI
- 23.34
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Kirby, E. N., Cohen, J. G., Guhathakurta, P., Cheng, L., Bullock, J. S., & Gallazzi, A. (2013). THE UNIVERSAL STELLAR MASS-STELLAR METALLICITY RELATION FOR DWARF GALAXIES. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/779/2/102
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