FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2802191161> ?p ?o ?g. }

• W2802191161 endingPage "112" @default.
• W2802191161 startingPage "97" @default.
• W2802191161 abstract "Recent observational studies of intermediate- and high-mass star-forming regions at submillimeter and infrared wavelengths are reviewed, and chemical diagnostics of the different physical components associated with young stellar objects are summarized. Procedures for determining the temperature, density and abundance profiles in the envelopes are outlined. A detailed study of a set of infrared-bright massive young stars reveals systematic increases in the gas/solid ratios, the abundances of evaporated molecules, and the fraction of heated ices with increasing temperature. Since these diverse phenomena involve a range of temperatures from < 100 K to 1000 K, the enhanced temperatures must be communicated to both the inner and outer parts of the envelopes. This ‘global heating’ plausibly results from the gradual dispersion of the envelopes with time. Similarities and differences with low-mass YSOs are discussed. The availability of accurate physical models will allow chemical models of ice evaporation followed by ‘hot core’ chemistry to be tested in detail." @default.
• W2802191161 created "2018-05-17" @default.
• W2802191161 creator A5048537056 @default.
• W2802191161 creator A5084364688 @default.
• W2802191161 date "2000-01-01" @default.
• W2802191161 modified "2023-09-25" @default.
• W2802191161 title "Chemistry in the Envelopes around Massive Young Stars" @default.
• W2802191161 cites W1488331733 @default.
• W2802191161 cites W1590758645 @default.
• W2802191161 cites W1978081588 @default.
• W2802191161 cites W1983103860 @default.
• W2802191161 cites W198330889 @default.
• W2802191161 cites W1985903255 @default.
• W2802191161 cites W1986387249 @default.
• W2802191161 cites W1993579535 @default.
• W2802191161 cites W1993677042 @default.
• W2802191161 cites W2000083902 @default.
• W2802191161 cites W2000541536 @default.
• W2802191161 cites W2003869289 @default.
• W2802191161 cites W2006521339 @default.
• W2802191161 cites W2009678133 @default.
• W2802191161 cites W2016136271 @default.
• W2802191161 cites W2022370015 @default.
• W2802191161 cites W2032204614 @default.
• W2802191161 cites W2033697868 @default.
• W2802191161 cites W2039381655 @default.
• W2802191161 cites W2040013037 @default.
• W2802191161 cites W2043802041 @default.
• W2802191161 cites W2050267833 @default.
• W2802191161 cites W2062437174 @default.
• W2802191161 cites W2063855687 @default.
• W2802191161 cites W2065434793 @default.
• W2802191161 cites W2071113235 @default.
• W2802191161 cites W2077235431 @default.
• W2802191161 cites W2078847722 @default.
• W2802191161 cites W2089737056 @default.
• W2802191161 cites W2095294995 @default.
• W2802191161 cites W2101651466 @default.
• W2802191161 cites W2127547331 @default.
• W2802191161 cites W2151316678 @default.
• W2802191161 cites W2170718234 @default.
• W2802191161 cites W2402831836 @default.
• W2802191161 cites W27497044 @default.
• W2802191161 cites W3103301773 @default.
• W2802191161 cites W4240595121 @default.
• W2802191161 doi "https://doi.org/10.1017/s007418090016471x" @default.
• W2802191161 hasPublicationYear "2000" @default.
• W2802191161 type Work @default.
• W2802191161 sameAs 2802191161 @default.
• W2802191161 citedByCount "11" @default.
• W2802191161 countsByYear W28021911612017 @default.
• W2802191161 crossrefType "journal-article" @default.
• W2802191161 hasAuthorship W2802191161A5048537056 @default.
• W2802191161 hasAuthorship W2802191161A5084364688 @default.
• W2802191161 hasBestOaLocation W28021911612 @default.
• W2802191161 hasConcept C120665830 @default.
• W2802191161 hasConcept C121332964 @default.
• W2802191161 hasConcept C125857072 @default.
• W2802191161 hasConcept C1276947 @default.
• W2802191161 hasConcept C150846664 @default.
• W2802191161 hasConcept C153294291 @default.
• W2802191161 hasConcept C158355884 @default.
• W2802191161 hasConcept C159467904 @default.
• W2802191161 hasConcept C180920033 @default.
• W2802191161 hasConcept C196939603 @default.
• W2802191161 hasConcept C23254167 @default.
• W2802191161 hasConcept C44870925 @default.
• W2802191161 hasConcept C505870484 @default.
• W2802191161 hasConcept C61441594 @default.
• W2802191161 hasConcept C6260449 @default.
• W2802191161 hasConcept C77077793 @default.
• W2802191161 hasConcept C86803240 @default.
• W2802191161 hasConcept C87355193 @default.
• W2802191161 hasConcept C98444146 @default.
• W2802191161 hasConceptScore W2802191161C120665830 @default.
• W2802191161 hasConceptScore W2802191161C121332964 @default.
• W2802191161 hasConceptScore W2802191161C125857072 @default.
• W2802191161 hasConceptScore W2802191161C1276947 @default.
• W2802191161 hasConceptScore W2802191161C150846664 @default.
• W2802191161 hasConceptScore W2802191161C153294291 @default.
• W2802191161 hasConceptScore W2802191161C158355884 @default.
• W2802191161 hasConceptScore W2802191161C159467904 @default.
• W2802191161 hasConceptScore W2802191161C180920033 @default.
• W2802191161 hasConceptScore W2802191161C196939603 @default.
• W2802191161 hasConceptScore W2802191161C23254167 @default.
• W2802191161 hasConceptScore W2802191161C44870925 @default.
• W2802191161 hasConceptScore W2802191161C505870484 @default.
• W2802191161 hasConceptScore W2802191161C61441594 @default.
• W2802191161 hasConceptScore W2802191161C6260449 @default.
• W2802191161 hasConceptScore W2802191161C77077793 @default.
• W2802191161 hasConceptScore W2802191161C86803240 @default.
• W2802191161 hasConceptScore W2802191161C87355193 @default.
• W2802191161 hasConceptScore W2802191161C98444146 @default.
• W2802191161 hasLocation W28021911611 @default.
• W2802191161 hasLocation W28021911612 @default.
• W2802191161 hasOpenAccess W2802191161 @default.
• W2802191161 hasPrimaryLocation W28021911611 @default.
• W2802191161 hasRelatedWork W1980800719 @default.

• next