Chemical and radiative transfer modelling of the ISO-LWS Fabry-Perot spectra of Orion-KL water lines

Monthly Notices of the Royal Astronomical Society

Volumn 406, Issue 4, 2010, Pages 2445-2451

  Lerate, M R ^a,b   Yates, J A ^a   Barlow, M J ^a   Viti, S ^a   Swinyard, B M ^c  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b EUROPEAN SPACE AGENCY   (Spain)

^c RUTHERFORD APPLETON LABORATORY   (United Kingdom)

Author keywords

Infrared: ISM; ISM: individual: Orion; ISM: lines and bands; ISM: molecules; Line: identification; Surveys

Indexed keywords

DENSITY OF GASES; FABRY-PEROT INTERFEROMETERS; WATER PIPING SYSTEMS;

FABRY-PEROT; INFRARED SPACE OBSERVATORY; INFRARED: ISM; ISM: INDIVIDUAL: ORION; ISM: INDIVIDUALS; ISM: LINE AND BANDS; ISM:MOLECULES; LINE:IDENTIFICATION; LONG WAVELENGTH SPECTROMETER; RADIATIVE TRANSFER MODELLING;

RADIATIVE TRANSFER;

EID: 77955345148     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16478.x     Document Type: Article

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