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WFRF:(Waters Michael F)
 

Sökning: WFRF:(Waters Michael F) > The chemical invent...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004285naa a2200781 4500
001oai:DiVA.org:su-221368
003SwePub
008230919s2023 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2213682 URI
024a https://doi.org/10.1039/d3fd00013c2 DOI
040 a (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Kamp, Inga4 aut
2451 0a The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program
264 1c 2023
338 a print2 rdacarrier
520 a The understanding of planet formation has changed recently, embracing the new idea of pebble accretion. This means that the influx of pebbles from the outer regions of planet-forming disks to their inner zones could determine the composition of planets and their atmospheres. The solid and molecular components delivered to the planet-forming region can be best characterized by mid-infrared spectroscopy. With Spitzer low-resolution (R = 100, 600) spectroscopy, this approach was limited to the detection of abundant molecules, such as H2O, C2H2, HCN and CO2. This contribution will present the first results of the MINDS (MIRI mid-INfrared Disk Survey, PI:Th Henning) project. Due do the sensitivity and spectral resolution provided by the James Webb Space Telescope (JWST), we now have a unique tool to obtain the full inventory of chemistry in the inner disks of solar-type stars and brown dwarfs, including also less-abundant hydrocarbons and isotopologues. The Integral Field Unit (IFU) capabilities will enable at the same time spatial studies of the continuum and line emission in extended sources such as debris disks, the flying saucer and also the search for mid-IR signatures of forming planets in systems such as PDS 70. These JWST observations are complementary to ALMA and NOEMA observations of outer-disk chemistry; together these datasets will provide an integral view of the processes occurring during the planet-formation phase.
650 7a NATURVETENSKAPx Kemix Annan kemi0 (SwePub)104992 hsv//swe
650 7a NATURAL SCIENCESx Chemical Sciencesx Other Chemistry Topics0 (SwePub)104992 hsv//eng
700a Henning, Thomas4 aut
700a Arabhavi, Aditya M.4 aut
700a Bettoni, Giulio4 aut
700a Christiaens, Valentin4 aut
700a Gasman, Danny4 aut
700a Grant, Sierra L.4 aut
700a Morales-Calderon, Maria4 aut
700a Tabone, Benoit4 aut
700a Abergel, Alain4 aut
700a Absil, Olivier4 aut
700a Argyriou, Ioannis4 aut
700a Barrado, David4 aut
700a Boccaletti, Anthony4 aut
700a Bouwman, Jeroen4 aut
700a Garatti, Alessio4 aut
700a van Dishoeck, Ewine F.4 aut
700a Geers, Vincent4 aut
700a Glauser, Adrian M.4 aut
700a Guedel, Manuel4 aut
700a Guadarrama, Rodrigo4 aut
700a Jang, Hyerin4 aut
700a Kanwar, Jayatee4 aut
700a Lagage, Pierre-Olivier4 aut
700a Lahuis, Fred4 aut
700a Mueller, Michael4 aut
700a Nehme, Cyrine4 aut
700a Olofsson, Göran,d 1944-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)olofsson
700a Pantin, Eric4 aut
700a Pawellek, Nicole4 aut
700a Perotti, Giulia4 aut
700a Ray, Tom P.4 aut
700a Rodgers-Lee, Donna4 aut
700a Samland, Matthias4 aut
700a Scheithauer, Silvia4 aut
700a Schreiber, Juergen4 aut
700a Schwarz, Kamber4 aut
700a Temmink, Milou4 aut
700a Vandenbussche, Bart4 aut
700a Vlasblom, Marissa4 aut
700a Waelkens, Christoffel4 aut
700a Waters, L. B. F. M.4 aut
700a Wright, Gillian4 aut
710a Stockholms universitetb Institutionen för astronomi4 org
773t Faraday discussionsg 245, s. 112-137q 245<112-137x 1359-6640x 1364-5498
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-221368
8564 8u https://doi.org/10.1039/d3fd00013c

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