the iras bright galaxy sample contains several moderate-luminosity galaxies exhibiting the similar iras spectra to those of cool ultraluminous infrared galaxies such as arp 220 (e.g., ngc 2623). namely, their infrared luminosities are less than 10^12 l(sun), and their iras spectra are nearly blackbody with color temperatures of 60-80 k (see figure). these moderate-luminosity blackbody-like infrared galaxies (mbigs) should be the early, dust-enshrouded stages in the evolution of seyfert/starburst galaxies. this is because most of mbigs are oh megamasers/absorbers, mergers, and/or show the enhanced ratios of the infrared luminosity to the molecular-gas mass. these are the properties characteristic of ultraluminous infrared galaxies, which are considered as the initial stages of quasars. therefore, the studies of mbigs will be essential to the complete understanding of seyfert/starburst phenomena, as in the case of ultraluminous infrared galaxies being crucial to the study of quasars. however, the dominant energy sources of mbigs are unknown. hence we propose the photo-s observation of mbigs. the main purpose is the measurement of the pah emission feature at 7.7 micron and the silicate absorption feature at 9.7 micron so as to determine the dominant energy sources (agns or ob stars). the pah features are useful in estimating the contribution from ob stars to the far-infrared luminosity. this is because (1) the pah features are excited by uv photons from ob stars, (2) the ratio of the number of the photons emitted in a certain pah feature to the total number of absorbed uv/optical photons is constant, and (3) pahs are destroyed by x-rays from agns. the 7.7 micron feature is stronger by a factor of 3-10 than the pah features observable from the ground. moreover, the reddening effect is very small at 7.7 micron. on the other hand, the depth of the silicate absorption feature is a measure of interstellar extinction. this kind of mid-infrared spectroscopy is available only with the advent of iso. in particular, photo-s is optimized for the investigations of pah features and the 9.7 micron absorption feature.
Instrument
PHT03 , PHT40
Temporal Coverage
1996-05-04T07:47:47Z/1996-08-26T08:38:14Z
Version
1.0
Mission Description
The Infrared Space Observatory (ISO) was the worlds first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
European Space Agency, Mouri et al., 1999, 'MIR Spectroscopy of Heavily Obscured IRAS Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-g54p6iy
