H(alpha) and Far-Infrared Emission Within the Early-Type Spiral Galaxy M81

Details H(alpha) and Far-Infrared Emission Within the Early-Type Spiral Galaxy M81 H(alpha) and Far-Infrared Emission Within the Early-Type Spiral Galaxy M81

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....111.2115d&link_type=abstract

Astronomical Journal v.111, p.2115

Astronomy and Astrophysics

Astronomy

5

Errata

Scientific paper

The S_100 micron_/S_60 micron_ color temperatures reported in Table I and depicted in Figs. 7,8, and 9 were inadvertently calculated using a λ^0^ emissivity law rather than the λ^-1^ emissivity law cited. Revised figures and a table listing the correct temperatures are provided below. The revision has affected the magnitude of the dust temperatures but not the location of the maxima and minima depicted in Fig. 2. The revised temperatures are about 4 K lower than originally reported. The bulge of M81 is still the hottest location but not by as large a margin. [See Journal].

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