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Interferometric CO observations of the ultraluminous IRAS galaxies ARP 220, IC 694/NGC 3690, NGC 6420 and NGC 7469

Authors :
Sargent, A. I
Sanders, D. B
Scoville, N. Z
Soifer, B. T
Source :
NASA, Washington Star Formation in Galaxies.
Publication Year :
1987
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1987.

Abstract

High resolution CO observations of the IRAS galaxies Arp 220, IC 694/NGC 3690, NGC 6240 and NGC 7469 were made with the Millimeter Wave Interferometer of the Owen Valley Radio Observatory. These yield spatial information on scales of 1 to 5 kpc and allow the separation of compact condensations from the more extended emission in the galaxies. In the case of the obviously interacting system IC 694/NGC 3690 the contributions of each component can be discerned. For that galaxy, and also for Arp 220, the unusually high lumonisities may be produced by nonthermal processes rather than by intense bursts of star formation.

Subjects

Subjects :
Astronomy

Details

Language :
English
Database :
NASA Technical Reports
Journal :
NASA, Washington Star Formation in Galaxies
Notes :
NSF AST-84-12473
Publication Type :
Report
Accession number :
edsnas.19870014898
Document Type :
Report