The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
LUMINOUS INFRARED GALAXIES
Abstract
▪ Abstract At luminosities above 10 11 [Formula: see text], infrared galaxies become the dominant population of extragalactic objects in the local Universe (z ≲ 0.3), being more numerous than optically selected starburst and Seyfert galaxies and quasi-stellar objects at comparable bolometric luminosity. The trigger for the intense infrared emission appears to be the strong interaction/merger of molecular gas-rich spirals, and the bulk of the infrared luminosity for all but the most luminous objects is due to dust heating from an intense starburst within giant molecular clouds. At the highest luminosities (L ir > 10 12 [Formula: see text]), nearly all objects appear to be advanced mergers powered by a mixture of circumnuclear starburst and active galactic nucleus energy sources, both of which are fueled by an enormous concentration of molecular gas that has been funneled into the merger nucleus. These ultraluminous infrared galaxies may represent an important stage in the formation of quasi-stellar objects and powerful radio galaxies. They may also represent a primary stage in the formation of elliptical galaxy cores, the formation of globular clusters, and the metal enrichment of the intergalactic medium.
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Citations
Cites
Toomre, A., & Toomre, J. (1972) · The Astrophysical Journal · doi:10.1086/151823 · Cited by 2,555
Cited by
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
Kennicutt, R. C. (1998) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.36.1.189 · Cited by 6,578
The Relationship between Stellar Light Distributions of Galaxies and Their Formation Histories
Conselice, C. J. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/375001 · Cited by 875
Structure and Formation of Elliptical and Spheroidal Galaxies
Bender, R. (2016) · doi:10.15781/t28g8fm0v · Cited by 555
Toward an Understanding of the Rapid Decline of the Cosmic Star Formation Rate
Bell, E. F., Papovich, C., Wolf, C., Le Floc’h, E., Caldwell, J. A. R., Barden, M., Egami, E., McIntosh, D. H., Meisenheimer, K., Perez‐Gonzalez, P. G., et al. (2005) · The Astrophysical Journal · doi:10.1086/429552 · Cited by 494
THE MAJOR AND MINOR GALAXY MERGER RATES AT z < 1.5
Lotz, J. M., Jonsson, P., Cox, T. J., Croton, D., Primack, J. R., Somerville, R. S., & Stewart, K. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/742/2/103 · Cited by 450
Metadata
- Authors
- Sanders, D. B., & Mirabel, I. F.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 1996-09
- Volume
- 34
- Issue
- 1
- Pages
- 749-792
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2168495929
- Cited by
- 2,786
- References
- 1
- FWCI
- 7.56
- Type
- journal article
- Language
- en
- Open access
- closed
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- Sanders, D. B., & Mirabel, I. F. (1996). LUMINOUS INFRARED GALAXIES. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.34.1.749
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
