The Near-IR Continuum Emission in the ISM of Galaxies

Details The Near-IR Continuum Emission in the ISM of Galaxies The Near-IR Continuum Emission in the ISM of Galaxies

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...198.0811l&link_type=abstract

American Astronomical Society, 198th AAS Meeting, #08.11; Bulletin of the American Astronomical Society, Vol. 33, p.798

Astronomy and Astrophysics

Astronomy

Scientific paper

Using the ISO spectroscopic data of a large sample of galaxies, we show
that gas-bearing galaxies generally have a near-IR continuum in excess
of their photospheric emission. We will discuss the spectroscopic
propeties of this continuum emission and argue that it arises from the
ISM of galaxies.

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