High-latitude dust and the 617 MHz-850 μm relation in NGC 5775

Monthly Notices of the Royal Astronomical Society

Volumn 340, Issue 1, 2003, Pages 269-274

  Brar, Rupinder Singh ^a   Irwin, Judith A ^a   Saikia, D J ^b  

^a QUEEN S UNIVERSITY   (Canada)

^b NATIONAL CENTRE FOR RADIO ASTROPHYSICS   (India)

Author keywords

Galaxies: haloes; Galaxies: individual: NGC 5775; Radio continuum: galaxies; Submillimetre

Indexed keywords

DUST; RADIO ASTRONOMY; RADIO TELESCOPES; SYNCHROTRON RADIATION;

BOLOMETER ARRAY; GALAXIES: INDIVIDUALS; GALAXY: INDIVIDUAL: NGC 5775; GALAXY:HALO; GIANT METREWAVE RADIO TELESCOPES; HIGH LATITUDES; RADIO CONTINUUM: GALAXIES; RADIO EMISSION; SPIRAL GALAXIES; SUBMILLIMETRE;

GALAXIES;

EID: 0142073882     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06301.x     Document Type: Article

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