ISO Observations of Hot Dust in the Nucleus of the S0 Galaxy NGC 3998

Details ISO Observations of Hot Dust in the Nucleus of the S0 Galaxy NGC 3998 ISO Observations of Hot Dust in the Nucleus of the S0 Galaxy NGC 3998

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.1103f&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #11.03; Bulletin of the American Astronomical Society, Vol. 28, p.1287

Astronomy and Astrophysics

Astronomy

Scientific paper

ISOCAM maps of the Seyfert 1 S0 galaxy NGC 3998 between 4.5microns and
15microns detect both extended emission from the bulge stars and strong
point source emission from the nucleus. The inner regions of NGC 3998
appear to contain a few thousand solar masses of warm ( ~ 200 K) dust,
probably associated with the AGN.

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