FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W13404212> ?p ?o ?g. }

• W13404212 abstract "The interstellar medium is enriched primarily by matter ejected from evolved low and intermediate mass stars. The outflows from these stars create a circumstellar envelope in which a rich gas-phase and dust-nucleation chemistry takes place. We observed the nearest carbon-rich evolved star, IRC+10216, using the PACS (55-210 {mu}m) and SPIRE (194-672 {mu}m) spectrometers on board Herschel. We find several tens of lines from SiS and SiO, including lines from the v=1 vibrational level. For SiS these transitions range up to J=124-123, corresponding to energies around 6700K, while the highest detectable transition is J=90-89 for SiO, which corresponds to an energy around 8400K. Both species trace the dust formation zone of IRC+10216, and the broad energy ranges involved in their detected transitions permit us to derive the physical properties of the gas and the particular zone in which each species has been formed. This allows us to check the accuracy of chemical thermodynamical equilibrium models and the suggested depletion of SiS and SiO due to accretion onto dust grains." @default.
• W13404212 created "2016-06-24" @default.
• W13404212 creator A5001925204 @default.
• W13404212 creator A5011159548 @default.
• W13404212 creator A5012932218 @default.
• W13404212 creator A5014296970 @default.
• W13404212 creator A5018324173 @default.
• W13404212 creator A5020573983 @default.
• W13404212 creator A5021226554 @default.
• W13404212 creator A5022404635 @default.
• W13404212 creator A5024793349 @default.
• W13404212 creator A5027029632 @default.
• W13404212 creator A5030700829 @default.
• W13404212 creator A5038532828 @default.
• W13404212 creator A5040267885 @default.
• W13404212 creator A5045682348 @default.
• W13404212 creator A5047049012 @default.
• W13404212 creator A5047390355 @default.
• W13404212 creator A5047686813 @default.
• W13404212 creator A5049454073 @default.
• W13404212 creator A5050256035 @default.
• W13404212 creator A5051014997 @default.
• W13404212 creator A5052182015 @default.
• W13404212 creator A5052603243 @default.
• W13404212 creator A5053672246 @default.
• W13404212 creator A5057655975 @default.
• W13404212 creator A5057771393 @default.
• W13404212 creator A5060096577 @default.
• W13404212 creator A5064190876 @default.
• W13404212 creator A5064517388 @default.
• W13404212 creator A5066349884 @default.
• W13404212 creator A5071675520 @default.
• W13404212 creator A5079423456 @default.
• W13404212 creator A5080770863 @default.
• W13404212 creator A5084180921 @default.
• W13404212 creator A5088374523 @default.
• W13404212 creator A5089500608 @default.
• W13404212 creator A5091326359 @default.
• W13404212 creator A5091335453 @default.
• W13404212 creator A5091670104 @default.
• W13404212 creator A5065313702 @default.
• W13404212 date "2010-05-25" @default.
• W13404212 modified "2023-10-06" @default.
• W13404212 title "Silicon in the dust formation zone of IRC +10216 as observed with PACS and SPIRE on board Herschel" @default.
• W13404212 hasPublicationYear "2010" @default.
• W13404212 type Work @default.
• W13404212 sameAs 13404212 @default.
• W13404212 citedByCount "4" @default.
• W13404212 countsByYear W134042122012 @default.
• W13404212 countsByYear W134042122018 @default.
• W13404212 crossrefType "journal-article" @default.
• W13404212 hasAuthorship W13404212A5001925204 @default.
• W13404212 hasAuthorship W13404212A5011159548 @default.
• W13404212 hasAuthorship W13404212A5012932218 @default.
• W13404212 hasAuthorship W13404212A5014296970 @default.
• W13404212 hasAuthorship W13404212A5018324173 @default.
• W13404212 hasAuthorship W13404212A5020573983 @default.
• W13404212 hasAuthorship W13404212A5021226554 @default.
• W13404212 hasAuthorship W13404212A5022404635 @default.
• W13404212 hasAuthorship W13404212A5024793349 @default.
• W13404212 hasAuthorship W13404212A5027029632 @default.
• W13404212 hasAuthorship W13404212A5030700829 @default.
• W13404212 hasAuthorship W13404212A5038532828 @default.
• W13404212 hasAuthorship W13404212A5040267885 @default.
• W13404212 hasAuthorship W13404212A5045682348 @default.
• W13404212 hasAuthorship W13404212A5047049012 @default.
• W13404212 hasAuthorship W13404212A5047390355 @default.
• W13404212 hasAuthorship W13404212A5047686813 @default.
• W13404212 hasAuthorship W13404212A5049454073 @default.
• W13404212 hasAuthorship W13404212A5050256035 @default.
• W13404212 hasAuthorship W13404212A5051014997 @default.
• W13404212 hasAuthorship W13404212A5052182015 @default.
• W13404212 hasAuthorship W13404212A5052603243 @default.
• W13404212 hasAuthorship W13404212A5053672246 @default.
• W13404212 hasAuthorship W13404212A5057655975 @default.
• W13404212 hasAuthorship W13404212A5057771393 @default.
• W13404212 hasAuthorship W13404212A5060096577 @default.
• W13404212 hasAuthorship W13404212A5064190876 @default.
• W13404212 hasAuthorship W13404212A5064517388 @default.
• W13404212 hasAuthorship W13404212A5065313702 @default.
• W13404212 hasAuthorship W13404212A5066349884 @default.
• W13404212 hasAuthorship W13404212A5071675520 @default.
• W13404212 hasAuthorship W13404212A5079423456 @default.
• W13404212 hasAuthorship W13404212A5080770863 @default.
• W13404212 hasAuthorship W13404212A5084180921 @default.
• W13404212 hasAuthorship W13404212A5088374523 @default.
• W13404212 hasAuthorship W13404212A5089500608 @default.
• W13404212 hasAuthorship W13404212A5091326359 @default.
• W13404212 hasAuthorship W13404212A5091335453 @default.
• W13404212 hasAuthorship W13404212A5091670104 @default.
• W13404212 hasBestOaLocation W134042121 @default.
• W13404212 hasConcept C121332964 @default.
• W13404212 hasConcept C150846664 @default.
• W13404212 hasConcept C180920033 @default.
• W13404212 hasConcept C181313176 @default.
• W13404212 hasConcept C190841160 @default.
• W13404212 hasConcept C196939603 @default.
• W13404212 hasConcept C2776368116 @default.
• W13404212 hasConcept C2776401274 @default.
• W13404212 hasConcept C44870925 @default.

• next