Eales, Stephen Anthony ![]() |
Abstract
The authors present observations made with the JPL/SISEX SWIR infrared array of two luminous IRAS galaxies. The observations of NGC 6240 showed the nucleus to have different structures at 1.25, 1.65, and 2.2 μm. The observations of the NGC 3690/IC 694 system disclosed a 2.2 μm double source at the centre of NGC 3690.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | University of Hawaii, Institute for Astronomy |
Related URLs: | |
Last Modified: | 24 Oct 2022 11:50 |
URI: | https://orca.cardiff.ac.uk/id/eprint/49501 |
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