FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2080774701> ?p ?o ?g. }

• W2080774701 endingPage "127" @default.
• W2080774701 startingPage "120" @default.
• W2080774701 abstract "We present new aperture synthesis CO maps of the Antennae (NGC 4038/39) obtained with the Caltech Millimeter Array. These sensitive images show molecular emission associated with the two nuclei and a partial ring of star formation to the west of NGC 4038, as well as revealing the large extent of the extranuclear region of star formation (the overlap region), which dominates the CO emission from this system. The largest molecular complexes have masses of × 108 M☉, typically an order of magnitude larger than the largest structures seen to date in more quiescent galaxy disks. The extremely red luminous star clusters identified previously with the Hubble Space Telescope are well correlated with the CO emission, which supports the conclusion that they are highly embedded young objects rather than old globular clusters. There is an excellent correlation between the CO emission and the 15 μm emission seen with the Infrared Space Observatory, particularly for the brightest regions. The most massive complexes in the overlap region have similar [Ne III]/[Ne II] ratios, which implies that all these regions are forming many massive stars. However, only the brightest mid-infrared peak shows strong, rising continuum emission longward of 10 μm, indicative of very small dust grains heated to high temperatures by their proximity to nearby luminous stars. Since these grains are expected to be removed rapidly from the immediate environment of the massive stars, it is possible that this region contains very young (<1 Myr) sites of star formation. Alternatively, fresh dust grains could be driven into the sphere of influence of the massive stars, perhaps by the bulk motions of two giant molecular complexes. The kinematics and morphology of the CO emission in this region provide some support for this second scenario." @default.
• W2080774701 created "2016-06-24" @default.
• W2080774701 creator A5000936421 @default.
• W2080774701 creator A5012045154 @default.
• W2080774701 creator A5046824037 @default.
• W2080774701 creator A5090280053 @default.
• W2080774701 date "2000-10-10" @default.
• W2080774701 modified "2023-09-25" @default.
• W2080774701 title "High‐Resolution Imaging of Molecular Gas and Dust in the Antennae (NGC 4038/39): Super Giant Molecular Complexes" @default.
• W2080774701 cites W1965941590 @default.
• W2080774701 cites W1967646461 @default.
• W2080774701 cites W1977334807 @default.
• W2080774701 cites W1992421412 @default.
• W2080774701 cites W1994703407 @default.
• W2080774701 cites W1996622138 @default.
• W2080774701 cites W1997972076 @default.
• W2080774701 cites W2007088574 @default.
• W2080774701 cites W2013926921 @default.
• W2080774701 cites W2023809198 @default.
• W2080774701 cites W2028741328 @default.
• W2080774701 cites W2042169845 @default.
• W2080774701 cites W2053032772 @default.
• W2080774701 cites W2060257508 @default.
• W2080774701 cites W2071981687 @default.
• W2080774701 cites W2088853013 @default.
• W2080774701 cites W2090395333 @default.
• W2080774701 cites W2131382718 @default.
• W2080774701 cites W2155122056 @default.
• W2080774701 cites W2168495929 @default.
• W2080774701 cites W2951408172 @default.
• W2080774701 cites W3101352865 @default.
• W2080774701 doi "https://doi.org/10.1086/309504" @default.
• W2080774701 hasPublicationYear "2000" @default.
• W2080774701 type Work @default.
• W2080774701 sameAs 2080774701 @default.
• W2080774701 citedByCount "124" @default.
• W2080774701 countsByYear W20807747012012 @default.
• W2080774701 countsByYear W20807747012013 @default.
• W2080774701 countsByYear W20807747012014 @default.
• W2080774701 countsByYear W20807747012015 @default.
• W2080774701 countsByYear W20807747012016 @default.
• W2080774701 countsByYear W20807747012017 @default.
• W2080774701 countsByYear W20807747012018 @default.
• W2080774701 countsByYear W20807747012019 @default.
• W2080774701 countsByYear W20807747012020 @default.
• W2080774701 countsByYear W20807747012021 @default.
• W2080774701 countsByYear W20807747012022 @default.
• W2080774701 countsByYear W20807747012023 @default.
• W2080774701 crossrefType "journal-article" @default.
• W2080774701 hasAuthorship W2080774701A5000936421 @default.
• W2080774701 hasAuthorship W2080774701A5012045154 @default.
• W2080774701 hasAuthorship W2080774701A5046824037 @default.
• W2080774701 hasAuthorship W2080774701A5090280053 @default.
• W2080774701 hasBestOaLocation W20807747011 @default.
• W2080774701 hasConcept C113461152 @default.
• W2080774701 hasConcept C121332964 @default.
• W2080774701 hasConcept C125857072 @default.
• W2080774701 hasConcept C1276947 @default.
• W2080774701 hasConcept C150846664 @default.
• W2080774701 hasConcept C44870925 @default.
• W2080774701 hasConcept C48393594 @default.
• W2080774701 hasConcept C86021447 @default.
• W2080774701 hasConcept C98444146 @default.
• W2080774701 hasConceptScore W2080774701C113461152 @default.
• W2080774701 hasConceptScore W2080774701C121332964 @default.
• W2080774701 hasConceptScore W2080774701C125857072 @default.
• W2080774701 hasConceptScore W2080774701C1276947 @default.
• W2080774701 hasConceptScore W2080774701C150846664 @default.
• W2080774701 hasConceptScore W2080774701C44870925 @default.
• W2080774701 hasConceptScore W2080774701C48393594 @default.
• W2080774701 hasConceptScore W2080774701C86021447 @default.
• W2080774701 hasConceptScore W2080774701C98444146 @default.
• W2080774701 hasIssue "1" @default.
• W2080774701 hasLocation W20807747011 @default.
• W2080774701 hasOpenAccess W2080774701 @default.
• W2080774701 hasPrimaryLocation W20807747011 @default.
• W2080774701 hasRelatedWork W1560590063 @default.
• W2080774701 hasRelatedWork W1590605944 @default.
• W2080774701 hasRelatedWork W1981321621 @default.
• W2080774701 hasRelatedWork W2995317516 @default.
• W2080774701 hasRelatedWork W3099229510 @default.
• W2080774701 hasRelatedWork W3102059507 @default.
• W2080774701 hasRelatedWork W3163083320 @default.
• W2080774701 hasRelatedWork W4298384704 @default.
• W2080774701 hasRelatedWork W4308191026 @default.
• W2080774701 hasRelatedWork W1636161128 @default.
• W2080774701 hasVolume "542" @default.
• W2080774701 isParatext "false" @default.
• W2080774701 isRetracted "false" @default.
• W2080774701 magId "2080774701" @default.
• W2080774701 workType "article" @default.