Mid-infrared imaging of WL 16: The spatial distribution of the hydrocarbon emission features

Monthly Notices of the Royal Astronomical Society

Volumn 299, Issue 4, 1998, Pages 1209-1214

  Moore, T J T ^a   Emerson, J P ^b   Skinner, C J ^c   Meixner, M M ^d   Arens, J F ^e   Jernigan, J G ^e  

^a LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^b QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^c STScI   (United States)

^d UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Circumstellar matter; Dust, extinction; Infrared: ISM: lines and bands; ISM: individual: WL 16; ISM: molecules; Stars: pre main sequence

Indexed keywords

DUST; LUMINANCE; MOLECULES; SILICATES; STARS; THERMOGRAPHY (IMAGING);

CIRCUMSTELLAR MATTERS; DUST EXTINCTIONS; DUST GRAINS; EMISSION FEATURES; HYDROCARBON EMISSION; INFRARED: ISM: LINES AND BANDS; ISM: INDIVIDUAL: WL 16; ISM: INDIVIDUALS; ISM:MOLECULES; STARS: PRE-MAIN SEQUENCE;

POLYCYCLIC AROMATIC HYDROCARBONS;

EID: 0042425185     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01883.x     Document Type: Review

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