ultraluminous infrared galaxies
GPTKB entity
Properties (48)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
galaxy
|
| gptkbp:are |
often studied in the context of galaxy evolution
important for understanding the early universe often compared to other galaxy types for research purposes important for understanding the role of feedback in galaxy formation often studied in relation to cosmic microwave background radiation associated with high star formation rates more luminous than 10^12 solar luminosities often associated with high metallicity often associated with starburst activity often detected in deep surveys often found in dense environments often found in merging or interacting systems often found in the early universe. often found in the vicinity of galaxy clusters often linked to the formation of globular clusters often the subject of multi-wavelength studies often used as tracers of cosmic evolution typically found at high redshifts important for understanding cosmic star formation rates important for understanding the lifecycle of galaxies important for understanding the relationship between galaxies and dark energy important for understanding the formation of massive galaxies studied_using_the_Hubble_Space_Telescope |
| gptkbp:can_be |
be analyzed for their chemical composition
be associated with outflows of gas and dust be detected in the far-infrared spectrum be detected in the submillimeter range be found in various environments be observed with radio telescopes be studied for their role in the cosmic web be used to probe the interstellar medium be used to study the effects of cosmic inflation contain active supermassive black holes exhibit complex morphologies be classified into different types based on their spectra show variability in their luminosity over time be studied through their gravitational lensing effects be used to test theories of galaxy formation and evolution be studied in the context of dark matter halo properties be used to investigate the role of environment in galaxy evolution |
| gptkbp:canBe |
contain large amounts of molecular gas
exhibit AGN activity host multiple star-forming regions |
| gptkbp:exhibits |
strong emission lines
|
| gptkbp:has |
high infrared luminosity
significant dust content |
| https://www.w3.org/2000/01/rdf-schema#label |
ultraluminous infrared galaxies
|