Water in protoplanetary disks
| Data(s) |
29/04/2014
|
|---|---|
| Resumo |
<p>Infrared water line emission from protoplanetary disks, recently observed by the Spitzer and Herschel space telescopes, is thought to trace the surface layer of the inner to outer regions of the disks. We have modelled the water abundance profile and line emission, especially focusing on the effects of dust size growth and turbulent mixing. Comparison between model calculations and observations suggests a small grain model with turbulent mixing is preferred. Copyright © International Astronomical Union 2014.</p> |
| Identificador |
http://dx.doi.org/10.1017/S1743921313012891 http://www.scopus.com/inward/record.url?scp=84899784303&partnerID=8YFLogxK |
| Idioma(s) |
eng |
| Publicador |
Cambridge University Press |
| Direitos |
info:eu-repo/semantics/restrictedAccess |
| Fonte |
Nomura , H , Walsh , C , Heinzeller , D & Millar , T J 2014 , Water in protoplanetary disks . in Proceedings of the International Astronomical Union: formation, detection, and characterization of extrasolar habitable planets . S293 edn , vol. 3 , Cambridge University Press , pp. 235-237 . DOI: 10.1017/S1743921313012891 |
| Palavras-Chave | #line: formation #molecular processes #planetary systems: protoplanetary disks #/dk/atira/pure/subjectarea/asjc/3100/3103 #Astronomy and Astrophysics |
| Tipo |
contributionToPeriodical |
