Matches in SemOpenAlex for { <https://semopenalex.org/work/W2794006095> ?p ?o ?g. }
- W2794006095 endingPage "2469" @default.
- W2794006095 startingPage "2455" @default.
- W2794006095 abstract "We present the results of an outflow and infall survey towards a distance limited sample of 31 massive star forming regions drawn from the RMS survey. The presence of young, active outflows is identified from SiO (8-7) emission and the infall dynamics are explored using HCO$^+$/H$^{13}$CO$^+$ (4-3) emission. We investigate if the infall and outflow parameters vary with source properties, exploring whether regions hosting potentially young active outflows show similarities or differences with regions harbouring more evolved, possibly momentum driven, fossil outflows. SiO emission is detected towards approximately 46% of the sources. When considering sources with and without an SiO detection (i.e. potentially active and fossil outflows respectively), only the $^{12}$CO outflow velocity shows a significant difference between samples, indicating SiO is more prevalent towards sources with higher outflow velocities. Furthermore, we find the SiO luminosity increases as a function of the Herschel 70$mu$m to WISE 22$mu$m flux ratio, suggesting the production of SiO is prevalent in younger, more embedded regions. Similarly, we find tentative evidence that sources with an SiO detection have a smaller bolometric luminosity-to-mass ratio, indicating SiO (8-7) emission is associated with potentially younger regions. We do not find a prevalence towards sources displaying signatures of infall in our sample. However, the higher energy HCO$^+$ transitions may not be the best suited tracer of infall at this spatial resolution in these regions." @default.
- W2794006095 created "2018-03-29" @default.
- W2794006095 creator A5019712147 @default.
- W2794006095 creator A5056772422 @default.
- W2794006095 creator A5074837101 @default.
- W2794006095 creator A5083546811 @default.
- W2794006095 creator A5085935969 @default.
- W2794006095 date "2018-03-19" @default.
- W2794006095 modified "2023-09-24" @default.
- W2794006095 title "Infall and outflow motions towards a sample of massive star-forming regions from the RMS survey" @default.
- W2794006095 cites W1521845223 @default.
- W2794006095 cites W1662110814 @default.
- W2794006095 cites W1934684304 @default.
- W2794006095 cites W1964867136 @default.
- W2794006095 cites W1966505877 @default.
- W2794006095 cites W1968137411 @default.
- W2794006095 cites W1991610844 @default.
- W2794006095 cites W2041730224 @default.
- W2794006095 cites W2045831346 @default.
- W2794006095 cites W2046014627 @default.
- W2794006095 cites W2050372348 @default.
- W2794006095 cites W2073961934 @default.
- W2794006095 cites W2075669073 @default.
- W2794006095 cites W2086764113 @default.
- W2794006095 cites W2087634628 @default.
- W2794006095 cites W2108220845 @default.
- W2794006095 cites W2114001902 @default.
- W2794006095 cites W2117237551 @default.
- W2794006095 cites W2119766797 @default.
- W2794006095 cites W2121700344 @default.
- W2794006095 cites W2123250083 @default.
- W2794006095 cites W2142693527 @default.
- W2794006095 cites W2156658280 @default.
- W2794006095 cites W2249971484 @default.
- W2794006095 cites W2275080503 @default.
- W2794006095 cites W2603740260 @default.
- W2794006095 cites W2949316013 @default.
- W2794006095 cites W3098218194 @default.
- W2794006095 cites W3099123091 @default.
- W2794006095 cites W3099643197 @default.
- W2794006095 cites W3099711861 @default.
- W2794006095 cites W3099922280 @default.
- W2794006095 cites W3100052132 @default.
- W2794006095 cites W3100106758 @default.
- W2794006095 cites W3101272077 @default.
- W2794006095 cites W3101516175 @default.
- W2794006095 cites W3102479806 @default.
- W2794006095 cites W3102565918 @default.
- W2794006095 cites W3102910330 @default.
- W2794006095 cites W3103163489 @default.
- W2794006095 cites W3103580270 @default.
- W2794006095 cites W3103994133 @default.
- W2794006095 cites W3104294372 @default.
- W2794006095 cites W3105125868 @default.
- W2794006095 cites W3105656078 @default.
- W2794006095 cites W3105873387 @default.
- W2794006095 cites W3105978887 @default.
- W2794006095 cites W3121641015 @default.
- W2794006095 cites W4293003757 @default.
- W2794006095 doi "https://doi.org/10.1093/mnras/sty701" @default.
- W2794006095 hasPublicationYear "2018" @default.
- W2794006095 type Work @default.
- W2794006095 sameAs 2794006095 @default.
- W2794006095 citedByCount "6" @default.
- W2794006095 countsByYear W27940060952019 @default.
- W2794006095 countsByYear W27940060952020 @default.
- W2794006095 countsByYear W27940060952021 @default.
- W2794006095 countsByYear W27940060952022 @default.
- W2794006095 countsByYear W27940060952023 @default.
- W2794006095 crossrefType "journal-article" @default.
- W2794006095 hasAuthorship W2794006095A5019712147 @default.
- W2794006095 hasAuthorship W2794006095A5056772422 @default.
- W2794006095 hasAuthorship W2794006095A5074837101 @default.
- W2794006095 hasAuthorship W2794006095A5083546811 @default.
- W2794006095 hasAuthorship W2794006095A5085935969 @default.
- W2794006095 hasBestOaLocation W27940060952 @default.
- W2794006095 hasConcept C121332964 @default.
- W2794006095 hasConcept C12287442 @default.
- W2794006095 hasConcept C125857072 @default.
- W2794006095 hasConcept C1276947 @default.
- W2794006095 hasConcept C150846664 @default.
- W2794006095 hasConcept C153294291 @default.
- W2794006095 hasConcept C191897082 @default.
- W2794006095 hasConcept C192562407 @default.
- W2794006095 hasConcept C44870925 @default.
- W2794006095 hasConcept C68709404 @default.
- W2794006095 hasConcept C86132830 @default.
- W2794006095 hasConcept C98444146 @default.
- W2794006095 hasConceptScore W2794006095C121332964 @default.
- W2794006095 hasConceptScore W2794006095C12287442 @default.
- W2794006095 hasConceptScore W2794006095C125857072 @default.
- W2794006095 hasConceptScore W2794006095C1276947 @default.
- W2794006095 hasConceptScore W2794006095C150846664 @default.
- W2794006095 hasConceptScore W2794006095C153294291 @default.
- W2794006095 hasConceptScore W2794006095C191897082 @default.
- W2794006095 hasConceptScore W2794006095C192562407 @default.
- W2794006095 hasConceptScore W2794006095C44870925 @default.
- W2794006095 hasConceptScore W2794006095C68709404 @default.