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机译:Dust, Ice, and Gas in Time (DIGIT) Herschel program first results: A full PACS-SED scan of the gas line emission in protostar DK Chamaeleontis
University of Texas at Austin, Department of Astronomy, 1 University Station C1400, Austin, TX 78712-0259, United States;
Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, Netherlands;
Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, Ster Voldgade 5-7, 1350 Copenhagen K., DenmarkMax Planck Institute for Astronomy, K?nigstuhl 17, 69117 Heidelberg, GermanyInstituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200D, 3001 Leuven, BelgiumAstronomy Department, University of California, Berkeley, CA 94720, United StatesLaboratoire d'Astrophysique de Grenoble, CNRS/Université Joseph Fourier (UMR5571), BP 53, 38041 Grenoble Cedex 9, FranceDepartment of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, United StatesCaltech, Division of Geological and Planetary Sciences, Mail Code 150-21, Pasadena, CA 91125, United StatesMax-Planck-Institut für Extraterrestriche Physik, Garching, GermanyNaval Research Laboratory, Code 7211, Washington, DC 20375, United StatesInstitute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, United StatesHerschel Science Centre, European Space Astronomy Centre (ESA), PO Box 78, 28691 Villanueva de la Ca?ada (Madrid), SpainDepartment of Astronomy and Space Science, Astrophysical Research Center for the Structure and Evolution of the Cosmos, Sejong University, Seoul 143-747, South KoreaHarvard-Smithsonian Center for Astrophysics, MS 78, 60 Garden Street, Cambridge, MA 02138, United States;
Astrochemistry; Circumstellar matter; Infrared: ISM; Stars: formation; Stars: protostars; Submillimeter: ISM;