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ISM Parameters in the Normal Galaxy NGC 5713We report ISO Long Wavelength Spectrometer (LWS) observations fo the Sbc(s) pec galaxy NGC 5713. We have obtained strong detections of the fine-structure forbidden transitions [C(sub ii)] 158(micro)m, [O(sub i)]63(micro)m, and [O(sub iii)] 88(micro)m, and significant upper limits for[N(sub ii)]122(micro)m, [O(sub iii)] 52(micro)m, and [N(sub iii)] 57(micro)m. We also detect the galaxy's dust continuum emission between 43 and 197 microns.
Document ID
20060036495
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Lord, S. D.
Malhotra, S.
Lim, T.
Helou, G.
Beichman, C. A.
Dinerstein, H.
Hollenbach, D. J.
Hunter, D. A.
Lo, K. Y.
Lu, N. Y.
Rubin, R. H.
Stacey, G. J.
Thronson, H. A., Jr.
Werner, M. W.
Date Acquired
August 23, 2013
Publication Date
January 1, 1996
Distribution Limits
Public
Copyright
Other
Keywords
galaxies NGC5713 ISM infrared spectroscopy

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