FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2167306626> ?p ?o ?g. }

• W2167306626 endingPage "L138" @default.
• W2167306626 startingPage "L135" @default.
• W2167306626 abstract "We present Chandra X-ray observations of the Hydra A cluster of galaxies, and we report the discovery of structure in the central 80 kpc of the cluster's X-ray-emitting gas. The most remarkable structures are depressions in the X-ray surface brightness, approximately 25-35 kpc in diameter, that are coincident with Hydra A's radio lobes. The depressions are nearly devoid of X-ray-emitting gas, and there is no evidence for shock-heated gas surrounding the radio lobes. We suggest that the gas within the surface brightness depressions was displaced as the radio lobes expanded subsonically, leaving cavities in the hot atmosphere. The gas temperature declines from 4 keV at 70 kpc to 3 keV in the inner 20 kpc of the brightest cluster galaxy (BCG), and the cooling time of the gas is approximately 600 Myr in the inner 10 kpc. These properties are consistent with the presence of an approximately 34 M middle dot in circle yr-1 cooling flow within a 70 kpc radius. Bright X-ray emission is present in the BCG surrounding a recently accreted disk of nebular emission and young stars. The star formation rate is commensurate with the cooling rate of the hot gas within the volume of the disk, although the sink for the material that may be cooling at larger radii remains elusive. A bright, unresolved X-ray source is present in the BCG's nucleus, coincident with the radio core. Its X-ray spectrum is consistent with a power law absorbed by a foreground NH approximately 4x1022 cm-2 column of hydrogen. This column is roughly consistent with the hydrogen column seen in absorption toward the less, similar24 pc diameter VLBA radio source. Apart from the point source, no evidence for excess X-ray absorption above the Galactic column is found." @default.
• W2167306626 created "2016-06-24" @default.
• W2167306626 creator A5001638250 @default.
• W2167306626 creator A5012635295 @default.
• W2167306626 creator A5019623396 @default.
• W2167306626 creator A5023354361 @default.
• W2167306626 creator A5043587706 @default.
• W2167306626 creator A5043871279 @default.
• W2167306626 creator A5048009535 @default.
• W2167306626 creator A5066289165 @default.
• W2167306626 creator A5073329735 @default.
• W2167306626 creator A5075767792 @default.
• W2167306626 creator A5084532778 @default.
• W2167306626 date "2000-05-10" @default.
• W2167306626 modified "2023-10-18" @default.
• W2167306626 title "[ITAL]Chandra[/ITAL] X-Ray Observations of the Hydra A Cluster: An Interaction between the Radio Source and the X-Ray–emitting Gas" @default.
• W2167306626 cites W1968628191 @default.
• W2167306626 cites W1985706855 @default.
• W2167306626 cites W1995144105 @default.
• W2167306626 cites W2011329288 @default.
• W2167306626 cites W2014027177 @default.
• W2167306626 cites W2018955174 @default.
• W2167306626 cites W2023897244 @default.
• W2167306626 cites W2030083850 @default.
• W2167306626 cites W2043553454 @default.
• W2167306626 cites W2056721760 @default.
• W2167306626 cites W2137909286 @default.
• W2167306626 cites W3101273468 @default.
• W2167306626 cites W3103675837 @default.
• W2167306626 doi "https://doi.org/10.1086/312662" @default.
• W2167306626 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/10813666" @default.
• W2167306626 hasPublicationYear "2000" @default.
• W2167306626 type Work @default.
• W2167306626 sameAs 2167306626 @default.
• W2167306626 citedByCount "537" @default.
• W2167306626 countsByYear W21673066262012 @default.
• W2167306626 countsByYear W21673066262013 @default.
• W2167306626 countsByYear W21673066262014 @default.
• W2167306626 countsByYear W21673066262015 @default.
• W2167306626 countsByYear W21673066262016 @default.
• W2167306626 countsByYear W21673066262017 @default.
• W2167306626 countsByYear W21673066262018 @default.
• W2167306626 countsByYear W21673066262019 @default.
• W2167306626 countsByYear W21673066262020 @default.
• W2167306626 countsByYear W21673066262021 @default.
• W2167306626 countsByYear W21673066262022 @default.
• W2167306626 countsByYear W21673066262023 @default.
• W2167306626 crossrefType "journal-article" @default.
• W2167306626 hasAuthorship W2167306626A5001638250 @default.
• W2167306626 hasAuthorship W2167306626A5012635295 @default.
• W2167306626 hasAuthorship W2167306626A5019623396 @default.
• W2167306626 hasAuthorship W2167306626A5023354361 @default.
• W2167306626 hasAuthorship W2167306626A5043587706 @default.
• W2167306626 hasAuthorship W2167306626A5043871279 @default.
• W2167306626 hasAuthorship W2167306626A5048009535 @default.
• W2167306626 hasAuthorship W2167306626A5066289165 @default.
• W2167306626 hasAuthorship W2167306626A5073329735 @default.
• W2167306626 hasAuthorship W2167306626A5075767792 @default.
• W2167306626 hasAuthorship W2167306626A5084532778 @default.
• W2167306626 hasBestOaLocation W21673066261 @default.
• W2167306626 hasConcept C121332964 @default.
• W2167306626 hasConcept C12241035 @default.
• W2167306626 hasConcept C125857072 @default.
• W2167306626 hasConcept C1276947 @default.
• W2167306626 hasConcept C150846664 @default.
• W2167306626 hasConcept C156055797 @default.
• W2167306626 hasConcept C164866538 @default.
• W2167306626 hasConcept C178635117 @default.
• W2167306626 hasConcept C199360897 @default.
• W2167306626 hasConcept C2779328170 @default.
• W2167306626 hasConcept C38652104 @default.
• W2167306626 hasConcept C41008148 @default.
• W2167306626 hasConcept C43481613 @default.
• W2167306626 hasConcept C44870925 @default.
• W2167306626 hasConcept C62520636 @default.
• W2167306626 hasConcept C91228026 @default.
• W2167306626 hasConcept C98444146 @default.
• W2167306626 hasConceptScore W2167306626C121332964 @default.
• W2167306626 hasConceptScore W2167306626C12241035 @default.
• W2167306626 hasConceptScore W2167306626C125857072 @default.
• W2167306626 hasConceptScore W2167306626C1276947 @default.
• W2167306626 hasConceptScore W2167306626C150846664 @default.
• W2167306626 hasConceptScore W2167306626C156055797 @default.
• W2167306626 hasConceptScore W2167306626C164866538 @default.
• W2167306626 hasConceptScore W2167306626C178635117 @default.
• W2167306626 hasConceptScore W2167306626C199360897 @default.
• W2167306626 hasConceptScore W2167306626C2779328170 @default.
• W2167306626 hasConceptScore W2167306626C38652104 @default.
• W2167306626 hasConceptScore W2167306626C41008148 @default.
• W2167306626 hasConceptScore W2167306626C43481613 @default.
• W2167306626 hasConceptScore W2167306626C44870925 @default.
• W2167306626 hasConceptScore W2167306626C62520636 @default.
• W2167306626 hasConceptScore W2167306626C91228026 @default.
• W2167306626 hasConceptScore W2167306626C98444146 @default.
• W2167306626 hasIssue "2" @default.
• W2167306626 hasLocation W21673066261 @default.
• W2167306626 hasLocation W21673066262 @default.
• W2167306626 hasLocation W21673066263 @default.

• next