Sökning: WFRF:(Floren H. G.) > The chemical compos...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 03583naa a2200517 4500 | |
001 | oai:research.chalmers.se:7871ce87-c57b-4196-a920-8c6c6193e0c2 | |
003 | SwePub | |
008 | 180103s2009 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-31444 | |
020 | a 9783540769583 | |
024 | 7 | a https://research.chalmers.se/publication/2542612 URI |
024 | 7 | a https://doi.org/10.1007/978-3-540-76959-0_322 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-314442 URI |
040 | a (SwePub)cthd (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a kon2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Crovisier, J.u Observatoire de Paris-Meudon4 aut |
245 | 1 0 | a The chemical composition of 9P/tempel 1 from radio observations |
264 | 1 | a Berlin, Heidelberg :b Springer Berlin Heidelberg,c 2009 |
520 | a In 2005, as part of a world-wide multi-wavelength investigation of comet 9P/Tempel 1 in support to the Deep Impact mission, we conducted radio spectroscopic observations with the Nançay radio telescope, the Odin satellite, the CSO 10-m and the IRAM 30-m telescopes. We report here our results concerning the chemical composition of the comet. The relative abundances of the detected species (H2O, CH3OH, H2S, HCN) or their upper limits (CO, H2CO, CS) are comparable to the mean values observed in other comets. No significant changes of the outgassing rates (except possibly for CH3OH) or of the molecular abundances were observed following the impact. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a Planetary system | |
700 | 1 | a Biver, N.u Observatoire de Paris-Meudon4 aut |
700 | 1 | a Bockelée-Morvan, D.u Observatoire de Paris-Meudon4 aut |
700 | 1 | a Boissier, J.u Observatoire de Paris-Meudon4 aut |
700 | 1 | a Colom, P.u Observatoire de Paris-Meudon4 aut |
700 | 1 | a Lecacheux, A.u Observatoire de Paris-Meudon4 aut |
700 | 1 | a Moreno, R.u Observatoire de Paris-Meudon4 aut |
700 | 1 | a Paubert, G.u Institut de Radioastronomie Millimétrique (IRAM)4 aut |
700 | 1 | a Lis, D. C.u California Institute of Technology (Caltech)4 aut |
700 | 1 | a Sumner, M.u California Institute of Technology (Caltech)4 aut |
700 | 1 | a Frisk, U.u Swedish Space Corporation (SSC)4 aut |
700 | 1 | a Hjalmarson, Åke,d 1939u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)akehjalm |
700 | 1 | a Olberg, Michael,d 1956u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)olberg |
700 | 1 | a Winnberg, Anders,d 1937u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)andwin |
700 | 1 | a Florén, H.-G.u Stockholms universitet,Institutionen för astronomi,Stockholm Observatory4 aut |
700 | 1 | a Sandqvist, A.u Stockholms universitet,Institutionen för astronomi,Stockholm Observatory4 aut |
700 | 1 | a Kwok, S.u Academia Sinica Taiwan,University of Calgary4 aut |
710 | 2 | a Observatoire de Paris-Meudonb Institut de Radioastronomie Millimétrique (IRAM)4 org |
773 | 0 | t ESO Astrophysics Symposiad Berlin, Heidelberg : Springer Berlin Heidelbergg 2009, s. 243-248q 2009<243-248x 1431-2433x 1611-6143z 9783540769583 |
856 | 4 8 | u https://research.chalmers.se/publication/254261 |
856 | 4 8 | u https://doi.org/10.1007/978-3-540-76959-0_32 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-31444 |
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