FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104392435> ?p ?o ?g. }

• W3104392435 endingPage "L28" @default.
• W3104392435 startingPage "L28" @default.
• W3104392435 abstract "We present first results from the Blind Ultra-Deep H i Environmental Survey of the Westerbork Synthesis Radio Telescope. Our survey is the first direct imaging study of neutral atomic hydrogen gas in galaxies at a redshift where evolutionary processes begin to show. In this Letter we investigate star formation, H i content, and galaxy morphology, as a function of environment in Abell 2192 (at z = 0.1876). Using a three-dimensional visualization technique, we find that Abell 2192 is a cluster in the process of forming, with significant substructure in it. We distinguish four structures that are separated in redshift and/or space. The richest structure is the baby cluster itself, with a core of elliptical galaxies that coincides with (weak) X-ray emission, almost no H i detections, and suppressed star formation. Surrounding the cluster, we find a compact group where galaxies pre-process before falling into the cluster, and a scattered population of field-like galaxies showing more star formation and H i detections. This cluster proves to be an excellent laboratory to understand the fate of the H i gas in the framework of galaxy evolution. We clearly see that the H i gas and the star formation correlate with morphology and environment at z ∼ 0.2. In particular, the fraction of H i detections is significantly affected by the environment. The effect starts to kick in in low-mass groups that pre-process the galaxies before they enter the cluster. Our results suggest that by the time the group galaxies fall into the cluster, they are already devoid of H i." @default.
• W3104392435 created "2020-11-23" @default.
• W3104392435 creator A5002757985 @default.
• W3104392435 creator A5041842578 @default.
• W3104392435 creator A5044660520 @default.
• W3104392435 creator A5061497047 @default.
• W3104392435 creator A5066509605 @default.
• W3104392435 date "2012-08-21" @default.
• W3104392435 modified "2023-10-16" @default.
• W3104392435 title "GAS RESERVOIRS AND STAR FORMATION IN A FORMING GALAXY CLUSTER AT <i>z</i> ⋍0.2" @default.
• W3104392435 cites W1609444141 @default.
• W3104392435 cites W1973086803 @default.
• W3104392435 cites W1977637580 @default.
• W3104392435 cites W1987922502 @default.
• W3104392435 cites W1989910526 @default.
• W3104392435 cites W2002284373 @default.
• W3104392435 cites W2033654844 @default.
• W3104392435 cites W2034933552 @default.
• W3104392435 cites W2035664515 @default.
• W3104392435 cites W2041335483 @default.
• W3104392435 cites W2042752995 @default.
• W3104392435 cites W2048758550 @default.
• W3104392435 cites W2055327934 @default.
• W3104392435 cites W2060673519 @default.
• W3104392435 cites W2063979326 @default.
• W3104392435 cites W2064056132 @default.
• W3104392435 cites W2075974992 @default.
• W3104392435 cites W2077005128 @default.
• W3104392435 cites W2085039857 @default.
• W3104392435 cites W2098488451 @default.
• W3104392435 cites W2115602332 @default.
• W3104392435 cites W2131462587 @default.
• W3104392435 cites W2148729646 @default.
• W3104392435 cites W3099490527 @default.
• W3104392435 cites W3099575556 @default.
• W3104392435 cites W3100294018 @default.
• W3104392435 cites W3100341048 @default.
• W3104392435 cites W3101440654 @default.
• W3104392435 cites W3102824424 @default.
• W3104392435 cites W3105142008 @default.
• W3104392435 cites W3105229970 @default.
• W3104392435 cites W4295846615 @default.
• W3104392435 cites W3105735649 @default.
• W3104392435 doi "https://doi.org/10.1088/2041-8205/756/2/l28" @default.
• W3104392435 hasPublicationYear "2012" @default.
• W3104392435 type Work @default.
• W3104392435 sameAs 3104392435 @default.
• W3104392435 citedByCount "37" @default.
• W3104392435 countsByYear W31043924352013 @default.
• W3104392435 countsByYear W31043924352014 @default.
• W3104392435 countsByYear W31043924352015 @default.
• W3104392435 countsByYear W31043924352016 @default.
• W3104392435 countsByYear W31043924352018 @default.
• W3104392435 countsByYear W31043924352019 @default.
• W3104392435 countsByYear W31043924352020 @default.
• W3104392435 countsByYear W31043924352021 @default.
• W3104392435 countsByYear W31043924352022 @default.
• W3104392435 countsByYear W31043924352023 @default.
• W3104392435 crossrefType "journal-article" @default.
• W3104392435 hasAuthorship W3104392435A5002757985 @default.
• W3104392435 hasAuthorship W3104392435A5041842578 @default.
• W3104392435 hasAuthorship W3104392435A5044660520 @default.
• W3104392435 hasAuthorship W3104392435A5061497047 @default.
• W3104392435 hasAuthorship W3104392435A5066509605 @default.
• W3104392435 hasBestOaLocation W31043924351 @default.
• W3104392435 hasConcept C121332964 @default.
• W3104392435 hasConcept C125857072 @default.
• W3104392435 hasConcept C1276947 @default.
• W3104392435 hasConcept C144024400 @default.
• W3104392435 hasConcept C149923435 @default.
• W3104392435 hasConcept C152268414 @default.
• W3104392435 hasConcept C156055797 @default.
• W3104392435 hasConcept C160147972 @default.
• W3104392435 hasConcept C164866538 @default.
• W3104392435 hasConcept C174802034 @default.
• W3104392435 hasConcept C199360897 @default.
• W3104392435 hasConcept C2908647359 @default.
• W3104392435 hasConcept C37119246 @default.
• W3104392435 hasConcept C41008148 @default.
• W3104392435 hasConcept C44870925 @default.
• W3104392435 hasConcept C871022 @default.
• W3104392435 hasConcept C98444146 @default.
• W3104392435 hasConceptScore W3104392435C121332964 @default.
• W3104392435 hasConceptScore W3104392435C125857072 @default.
• W3104392435 hasConceptScore W3104392435C1276947 @default.
• W3104392435 hasConceptScore W3104392435C144024400 @default.
• W3104392435 hasConceptScore W3104392435C149923435 @default.
• W3104392435 hasConceptScore W3104392435C152268414 @default.
• W3104392435 hasConceptScore W3104392435C156055797 @default.
• W3104392435 hasConceptScore W3104392435C160147972 @default.
• W3104392435 hasConceptScore W3104392435C164866538 @default.
• W3104392435 hasConceptScore W3104392435C174802034 @default.
• W3104392435 hasConceptScore W3104392435C199360897 @default.
• W3104392435 hasConceptScore W3104392435C2908647359 @default.
• W3104392435 hasConceptScore W3104392435C37119246 @default.
• W3104392435 hasConceptScore W3104392435C41008148 @default.
• W3104392435 hasConceptScore W3104392435C44870925 @default.
• W3104392435 hasConceptScore W3104392435C871022 @default.

• next