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.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...315l..75k&link_type=abstract

Astronomy and Astrophysics, v.315, p.L75-L78

Astronomy and Astrophysics

Astrophysics

16

Galaxies: Elliptical And Lenticular, Cd, Galaxies: Individual: Ngc 3998, Galaxies: Ism, Galaxies: Seyfert

Scientific paper

ISOCAM maps of the Seyfert 1 S0 galaxy NGC 3998 between 4.5μm and
15μm 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 (~200K) dust,
probably associated with the AGN.

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