FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2040147953> ?p ?o ?g. }

• W2040147953 endingPage "146" @default.
• W2040147953 startingPage "123" @default.
• W2040147953 abstract "We present J (1.2 microns) H (1-6 microns) K' (2.11 microns) and Br(gamma) (2.166 microns) images from four large regions within the central 40 pc of the Galaxy. Localized variations in the extinction, as determined by observations of the stellar population, are examined using the median H-K' color as a function of position within each region. As the value of the derived extinction from the stars is dependent upon the intrinsic magnitude of the assumed stellar type, the J-H vs. H-K' diagrams are first used to investigate the distribution of stellar types in the four regions. We find that there is a distinct OB population, contrary to earlier assumptions, with the ratio of K and M giants and supergiants to OB stars approximately twice that of the solar neighborhood. Although the on the scale of approx. 1 min. fluctuations in the extinction are on the order of A(sub V) approx. greater than 2, throughout the entire region the extinction varies from A(sub V) approx. greater than 25 to A(sub V) approx. less than 40. We also examine whether there is any variation in the extinction and stellar number density relative to the unusual radio features in these regions and do not find a significant correlation. Spectral imaging in Br(gamma) 2.166 microns emission shows a strong morphological correspondence between the 6 cm radio images and the diffuse Br(gamma) emission. By comparing the theoretical Br(gamma) flux derived from the radio flux using recombination theory, with our measured Br(gamma) flux, we obtain a second, independent, estimate of the extinction. We compare the two data sets and find that the extinction as derived from the stars is consistently greater, sometimes by a factor of two, than the value of the extinction derived from the Br(gamma) images. The derived extinction in various regions, however, is insufficient for any of these regions to be located behind the molecular clouds as previously observed in the Galactic Center, consistent with the theory that the observed radio emission is produced on the foreground surface of these clouds." @default.
• W2040147953 created "2016-06-24" @default.
• W2040147953 creator A5007052151 @default.
• W2040147953 creator A5025766906 @default.
• W2040147953 creator A5041068889 @default.
• W2040147953 creator A5049283549 @default.
• W2040147953 creator A5051539645 @default.
• W2040147953 creator A5089090678 @default.
• W2040147953 date "2000-07-01" @default.
• W2040147953 modified "2023-09-23" @default.
• W2040147953 title "Interstellar Extinction in the Vicinity of the Galactic Center" @default.
• W2040147953 cites W1568434795 @default.
• W2040147953 cites W1642684771 @default.
• W2040147953 cites W1967219221 @default.
• W2040147953 cites W1969449809 @default.
• W2040147953 cites W1971014210 @default.
• W2040147953 cites W1973276114 @default.
• W2040147953 cites W1977152037 @default.
• W2040147953 cites W1979224021 @default.
• W2040147953 cites W1981525549 @default.
• W2040147953 cites W1985403173 @default.
• W2040147953 cites W1988016384 @default.
• W2040147953 cites W1988798166 @default.
• W2040147953 cites W1989654624 @default.
• W2040147953 cites W1991040067 @default.
• W2040147953 cites W1991649159 @default.
• W2040147953 cites W1997972076 @default.
• W2040147953 cites W2002996080 @default.
• W2040147953 cites W2010481367 @default.
• W2040147953 cites W2010993162 @default.
• W2040147953 cites W2011491298 @default.
• W2040147953 cites W2013535230 @default.
• W2040147953 cites W2021194112 @default.
• W2040147953 cites W2024451778 @default.
• W2040147953 cites W2026795906 @default.
• W2040147953 cites W2027131240 @default.
• W2040147953 cites W2034702996 @default.
• W2040147953 cites W2057310326 @default.
• W2040147953 cites W2058937012 @default.
• W2040147953 cites W2061845514 @default.
• W2040147953 cites W2081087406 @default.
• W2040147953 cites W2081911925 @default.
• W2040147953 cites W2085441363 @default.
• W2040147953 cites W2086303799 @default.
• W2040147953 cites W2093172397 @default.
• W2040147953 cites W2094142265 @default.
• W2040147953 cites W2313890056 @default.
• W2040147953 cites W2331175717 @default.
• W2040147953 cites W2465945632 @default.
• W2040147953 cites W3011090980 @default.
• W2040147953 cites W4237816935 @default.
• W2040147953 cites W4244818491 @default.
• W2040147953 doi "https://doi.org/10.1086/313401" @default.
• W2040147953 hasPublicationYear "2000" @default.
• W2040147953 type Work @default.
• W2040147953 sameAs 2040147953 @default.
• W2040147953 citedByCount "32" @default.
• W2040147953 countsByYear W20401479532013 @default.
• W2040147953 countsByYear W20401479532017 @default.
• W2040147953 countsByYear W20401479532018 @default.
• W2040147953 countsByYear W20401479532019 @default.
• W2040147953 crossrefType "journal-article" @default.
• W2040147953 hasAuthorship W2040147953A5007052151 @default.
• W2040147953 hasAuthorship W2040147953A5025766906 @default.
• W2040147953 hasAuthorship W2040147953A5041068889 @default.
• W2040147953 hasAuthorship W2040147953A5049283549 @default.
• W2040147953 hasAuthorship W2040147953A5051539645 @default.
• W2040147953 hasAuthorship W2040147953A5089090678 @default.
• W2040147953 hasBestOaLocation W20401479532 @default.
• W2040147953 hasConcept C101991246 @default.
• W2040147953 hasConcept C120665830 @default.
• W2040147953 hasConcept C121332964 @default.
• W2040147953 hasConcept C1276947 @default.
• W2040147953 hasConcept C132552067 @default.
• W2040147953 hasConcept C196939603 @default.
• W2040147953 hasConcept C44870925 @default.
• W2040147953 hasConcept C98444146 @default.
• W2040147953 hasConceptScore W2040147953C101991246 @default.
• W2040147953 hasConceptScore W2040147953C120665830 @default.
• W2040147953 hasConceptScore W2040147953C121332964 @default.
• W2040147953 hasConceptScore W2040147953C1276947 @default.
• W2040147953 hasConceptScore W2040147953C132552067 @default.
• W2040147953 hasConceptScore W2040147953C196939603 @default.
• W2040147953 hasConceptScore W2040147953C44870925 @default.
• W2040147953 hasConceptScore W2040147953C98444146 @default.
• W2040147953 hasIssue "1" @default.
• W2040147953 hasLocation W20401479531 @default.
• W2040147953 hasLocation W20401479532 @default.
• W2040147953 hasLocation W20401479533 @default.
• W2040147953 hasOpenAccess W2040147953 @default.
• W2040147953 hasPrimaryLocation W20401479531 @default.
• W2040147953 hasRelatedWork W1922699913 @default.
• W2040147953 hasRelatedWork W2002418785 @default.
• W2040147953 hasRelatedWork W2018460911 @default.
• W2040147953 hasRelatedWork W2037983614 @default.
• W2040147953 hasRelatedWork W2618549331 @default.
• W2040147953 hasRelatedWork W3098997918 @default.
• W2040147953 hasRelatedWork W3102549633 @default.

• next