Cool dust and gas in the small magellanic cloud

Monthly Notices of the Royal Astronomical Society

Volumn 315, Issue 4, 2000, Pages 791-807

  Stanimirovic, S ^a,b,g   Staveley Smith, L ^b   Van Der Hulst, J M ^c   Bontekoe, Tj R ^d,e   Kester, D J M ^f   Jones, P A ^a  

^a UNIVERSITY OF WESTERN SYDNEY   (Australia)

^b CSIRO   (Australia)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

^d Bontekoe Data Consultancy   (Netherlands)

^e UNIVERSITY OF AMSTERDAM   (Netherlands)

^f SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^g ARECIBO OBSERVATORY   (Puerto Rico)

Author keywords

Dust; Extinction; Infrared: galaxies; ISM: clouds; Magellanic clouds

Indexed keywords

ASTRONOMICAL SATELLITES; DUST; HYDROGEN; INFRARED IMAGING; POWER SPECTRUM; STARS;

COLUMN DENSITY; EXTINCTION; FAR INFRARED; GAS RATIO; HIGH ANGULAR RESOLUTIONS; INFRARED GALAXIES; ISM : CLOUDS; LARGE AMOUNTS; MAGELLANIC CLOUDS; SMALL MAGELLANIC CLOUDS;

GALAXIES;

EID: 0001558358     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03480.x     Document Type: Article

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