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- Warm–hot_intergalactic_medium abstract "The warm–hot intergalactic medium (WHIM) refers to a sparse, warm-to-hot (105 to 107 K) plasma that cosmologists believe to exist in the spaces between galaxies and to contain 40–50% of the baryons (that is, 'normal matter' which exists as plasma or as atoms and molecules, in contrast to dark matter) in the universe at the current epoch. Because of the high temperature of the medium, the expectation is that it is most easily observed from the ultraviolet and low energy X-ray emission. Within the WHIM, gas shocks are created as a result of active galactic nuclei, along with the gravitationally-driven processes of merging and accretion. Part of the gravitational energy supplied by these effects is converted into thermal emissions of the matter by collisionless shock heating.In May 2010 a giant reservoir of WHIM was detected by the Chandra X-ray Observatory lying along the wall shaped structure of galaxies (Sculptor Wall) some 400 million light-years from Earth.".
- Warm–hot_intergalactic_medium wikiPageID "22689597".
- Warm–hot_intergalactic_medium wikiPageLength "2298".
- Warm–hot_intergalactic_medium wikiPageOutDegree "19".
- Warm–hot_intergalactic_medium wikiPageRevisionID "662942971".
- Warm–hot_intergalactic_medium wikiPageWikiLink Active_galactic_nucleus.
- Warm–hot_intergalactic_medium wikiPageWikiLink Atom.
- Warm–hot_intergalactic_medium wikiPageWikiLink Baryon.
- Warm–hot_intergalactic_medium wikiPageWikiLink Category:Intergalactic_media.
- Warm–hot_intergalactic_medium wikiPageWikiLink Chandra_X-ray_Observatory.
- Warm–hot_intergalactic_medium wikiPageWikiLink Chronology_of_the_universe.
- Warm–hot_intergalactic_medium wikiPageWikiLink Collisionless.
- Warm–hot_intergalactic_medium wikiPageWikiLink Cosmology.
- Warm–hot_intergalactic_medium wikiPageWikiLink Dark_matter.
- Warm–hot_intergalactic_medium wikiPageWikiLink Epoch_(cosmology).
- Warm–hot_intergalactic_medium wikiPageWikiLink Galaxy.
- Warm–hot_intergalactic_medium wikiPageWikiLink Gravitational_energy.
- Warm–hot_intergalactic_medium wikiPageWikiLink Intergalactic_medium.
- Warm–hot_intergalactic_medium wikiPageWikiLink Intracluster_medium.
- Warm–hot_intergalactic_medium wikiPageWikiLink Light-year.
- Warm–hot_intergalactic_medium wikiPageWikiLink Light-years.
- Warm–hot_intergalactic_medium wikiPageWikiLink Molecule.
- Warm–hot_intergalactic_medium wikiPageWikiLink Outer_space.
- Warm–hot_intergalactic_medium wikiPageWikiLink Plasma_(physics).
- Warm–hot_intergalactic_medium wikiPageWikiLink Sculptor_Wall.
- Warm–hot_intergalactic_medium wikiPageWikiLink Shock_heating.
- Warm–hot_intergalactic_medium wikiPageWikiLink Shock_wave.
- Warm–hot_intergalactic_medium wikiPageWikiLink Shock_waves_in_astrophysics.
- Warm–hot_intergalactic_medium wikiPageWikiLinkText "Intergalactic medium".
- Warm–hot_intergalactic_medium wikiPageWikiLinkText "Warm–hot intergalactic medium".
- Warm–hot_intergalactic_medium wikiPageWikiLinkText "space between galaxies".
- Warm–hot_intergalactic_medium wikiPageWikiLinkText "warm–hot intergalactic medium".
- Warm–hot_intergalactic_medium hasPhotoCollection Warm–hot_intergalactic_medium.
- Warm–hot_intergalactic_medium wikiPageUsesTemplate Template:Astronomy-stub.
- Warm–hot_intergalactic_medium wikiPageUsesTemplate Template:Reflist.
- Warm–hot_intergalactic_medium wikiPageUsesTemplate Template:Wiktionary.
- Warm–hot_intergalactic_medium subject Category:Intergalactic_media.
- Warm–hot_intergalactic_medium comment "The warm–hot intergalactic medium (WHIM) refers to a sparse, warm-to-hot (105 to 107 K) plasma that cosmologists believe to exist in the spaces between galaxies and to contain 40–50% of the baryons (that is, 'normal matter' which exists as plasma or as atoms and molecules, in contrast to dark matter) in the universe at the current epoch. Because of the high temperature of the medium, the expectation is that it is most easily observed from the ultraviolet and low energy X-ray emission.".
- Warm–hot_intergalactic_medium label "Warm–hot intergalactic medium".
- Warm–hot_intergalactic_medium sameAs Warm-Hot_Intergalactic_Medium.
- Warm–hot_intergalactic_medium sameAs m.05zygdx.
- Warm–hot_intergalactic_medium sameAs Q593354.
- Warm–hot_intergalactic_medium sameAs Q593354.
- Warm–hot_intergalactic_medium wasDerivedFrom Warm–hot_intergalactic_medium?oldid=662942971.
- Warm–hot_intergalactic_medium isPrimaryTopicOf Warm–hot_intergalactic_medium.