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Searching for Cool Dust in the Mid-to-far Infrared: The Mass-loss Histories of the Hypergiants µ Cep, VY CMa, IRC+10420, and ρ Cas
DOI: 10.3847/0004-6256/151/3/51 Bibcode: 2016AJ....151...51S

Gehrz, Robert D.; Humphreys, Roberta M.; Jones, Terry J. +6 more

We present mid- and far-IR imaging of four famous hypergiant stars: the red supergiants µ Cep and VY CMa, and the warm hypergiants IRC +10420 and ρ Cas. Our 11-37 µm SOFIA/FORCAST imaging probes cool dust not detected in visual and near-IR imaging studies. Adaptive optics 8-12 µm imaging of µ Cep and IRC +10420 with MMT/MIR…

2016 The Astronomical Journal
AKARI Herschel ISO 55
Modeling of the Zodiacal Emission for the AKARI/IRC Mid-infrared All-sky Diffuse Maps
DOI: 10.3847/0004-6256/151/3/71 Bibcode: 2016AJ....151...71K

Onaka, Takashi; Ootsubo, Takafumi; Kaneda, Hidehiro +6 more

The zodiacal emission, which is the thermal infrared (IR) emission from the interplanetary dust (IPD) in our solar system, has been studied for a long time. Nevertheless, accurate modeling of the zodiacal emission has not been successful to reproduce the all-sky spatial distribution of the zodiacal emission, especially in the mid-IR where the zodi…

2016 The Astronomical Journal
AKARI 20
AKARI/IRC Near-infrared Spectral Atlas of Galactic Planetary Nebulae
DOI: 10.3847/0004-6256/151/4/93 Bibcode: 2016AJ....151...93O

Onaka, Takashi; Matsuura, Mikako; Sakon, Itsuki +2 more

Near-infrared (2.5-5.0 µm) low-resolution (λ/Δλ ∼ 100) spectra of 72 Galactic planetary nebulae (PNe) were obtained with the Infrared Camera (IRC) in the post-helium phase. The IRC, equipped with a 1‧ × 1‧ window for spectroscopy of a point source, was capable of obtaining near-infrared spectra in a slit-less mode without any flux loss due t…

2016 The Astronomical Journal
AKARI 16