Search Publications

Survey of Ices toward Massive Young Stellar Objects. I. OCS, CO, OCN-, and CH3OH
DOI: 10.3847/1538-4357/ac9b4a Bibcode: 2022ApJ...941...32B

Boogert, A. C. A.; Brewer, K.; Brittain, A. +1 more

An important tracer of the origin and evolution of cometary ices is the comparison with ices found in dense clouds and toward young stellar objects (YSOs). We present a survey of ices in the 2-5 µm spectra of 23 massive YSOs, taken with the NASA InfraRed Telescope Facility SpeX spectrometer. The 4.90 µm absorption band of OCS ice is de…

2022 The Astrophysical Journal
ISO 26
Bridging Optical and Far-infrared Emission-line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O III] 88 µm/SFR at z > 6
DOI: 10.3847/1538-4357/ac7fed Bibcode: 2022ApJ...935..119S

Harikane, Yuichi; Inoue, Akio K.; Hashimoto, Takuya +3 more

We present photoionization modeling of galaxy populations at z ∼ 0, 2, and >6 to bridge optical and far-infrared (FIR) emission-line diagrams. We collect galaxies with measurements of optical and/or FIR ([O III] 88 µm and [C II] 158 µm) emission-line fluxes and plot them on the [O III]λ5007/Hβ-[N II]λ6585/Hα (BPT) and L([O III]

2022 The Astrophysical Journal
Herschel ISO 17
SOFIA Observations of Far-IR Fine-structure Lines in Galaxies to Measure Metallicity
DOI: 10.3847/1538-4357/ac37b7 Bibcode: 2022ApJ...926...55S

Spinoglio, Luigi; Fernández-Ontiveros, Juan Antonio; Malkan, Matthew A. +8 more

We present new and archival SOFIA FIFI-LS far-IR spectroscopic observations of the [O III] 52 µm and/or the [N III] 57 µm lines of 25 local galaxies. Including 31 other galaxies from Herschel-PACS, we discuss a local sample of 47 galaxies, including the H II galaxies, luminous IR galaxies, low-metallicity dwarfs, and Seyfert nuclei. An…

2022 The Astrophysical Journal
Herschel ISO 16
[C II] Map of the Molecular Ring and Arms of the Spiral Galaxy NGC 7331
DOI: 10.3847/1538-4357/ac4252 Bibcode: 2022ApJ...926...82S

Fadda, Dario; Sutter, Jessica

We present the [C II] 157.7 µm map of galaxy NGC 7331 obtained with the Field-Imaging Far-Infrared Line Spectrometer on board the Stratospheric Observatory for Infrared Astronomy (SOFIA). This map extends an existent Herschel/Photodetector Array Camera and Spectrometer observation of the central strip of the galaxy to encompass the entire mo…

2022 The Astrophysical Journal
Herschel ISO 11
The Extremely Buried Nucleus of IRAS 17208-0014 Observed at Submillimeter and Near-infrared Wavelengths
DOI: 10.3847/1538-4357/ac57c2 Bibcode: 2022ApJ...928..184B

Onishi, Shusuke; Nakagawa, Takao; Baba, Shunsuke +6 more

The ultraluminous infrared galaxy IRAS 17208-0014 is a late-stage merger that hosts a buried active galactic nucleus (AGN). To investigate its nuclear structure, we performed high-spatial-resolution ( ~ 0.″04 ~ 32 pc) Atacama Large Millimeter/submillimeter Array (ALMA) observations in Band 9 (~450 µm or ~660 GHz), along with near-infrared AK…

2022 The Astrophysical Journal
AKARI Herschel ISO 10
Detection of the S(1) Rotational Line of H2 toward IRC+10216: A Simultaneous Measurement of the Mass-loss Rate and CO Abundance
DOI: 10.3847/2041-8213/ac5a58 Bibcode: 2022ApJ...927L..33F

Cernicharo, J.; Fonfría, J. P.; Richter, M. J. +2 more

We report the first detection of the S(1) pure rotational line of ortho-H2 at 17.04 µm in an asymptotic giant branch star, using observations of IRC+10216 with the Echelon-cross-echelle Spectrograph (EXES) mounted on the Stratospheric Observatory for Infrared Astronomy. This line, which was observed in a very high-sensitivity spec…

2022 The Astrophysical Journal
ISO 5
Detection of a Broad 8 µm UIR Feature in the Mid-infrared Spectrum of WR 125 Observed with Subaru/COMICS
DOI: 10.3847/1538-4357/ac63bd Bibcode: 2022ApJ...930..116E

Onaka, Takashi; Sakon, Itsuki; Williams, Peredur M. +3 more

We present the detection of a broad 8 µm feature in newly formed dust around the carbon-rich Wolf-Rayet (WC) binary WR 125 from N-band low-resolution (NL; R ~ 250) spectroscopy between 7.3 and 13.6 µm and N-band (11.7 µm) and Q-band (18.8 µm) imaging with Subaru/COMICS in 2019 October. WR 125 is a colliding-wind binary (WC7…

2022 The Astrophysical Journal
AKARI ISO 5
H1821+643: The Most X-Ray and Infrared Luminous Active Galactic Nucleus (AGN) in the Swift/BAT Survey in the Process of Rapid Stellar and Supermassive Black Hole Mass Assembly
DOI: 10.3847/1538-4357/ac9304 Bibcode: 2022ApJ...940....7F

Hashimoto, Takuya; Ricci, Claudio; Izumi, Takuma +6 more

H1821+643 is the most X-ray luminous nonbeamed active galactic nucleus (AGN) of L 14-150 keV = 5.2 × 1045 erg s-1 in the Swift/Burst Alert Telescope (BAT) ultrahard X-ray survey, and it is also a hyperluminous infrared (IR) galaxy L IR = 1013.2 L residing in the center of a massiv…

2022 The Astrophysical Journal
AKARI ISO eHST 3
Toward Understanding the B[e] Phenomenon. VIII. Nature and Variability of IRAS 07080+0605
DOI: 10.3847/1538-4357/ac6de0 Bibcode: 2022ApJ...932...36K

Miroshnichenko, A. S.; Manset, N.; Zharikov, S. V. +13 more

We report the results of spectroscopic and photometric observations of the emission-line object IRAS 07080+0605 carried out in 2004-2021. We found that the object is significantly underluminous for its spectroscopic properties (T eff = 8500 ± 500 K, $\mathrm{log}$ g = 2.0 ± 0.5), if a strong visual attenuation by a factor of ~43 found t…

2022 The Astrophysical Journal
AKARI Gaia ISO 1
SOFIA/FORCAST Monitoring of the Dust Emission from R Aqr: Start of the Eclipse
DOI: 10.3847/1538-4357/ac4792 Bibcode: 2022ApJ...926..177S

Gorti, Uma; Whitelock, Patricia A.; Wagner, R. Mark +3 more

We present mid-infrared (mid-IR) spectra from our continued monitoring of R Aquarii, the nearest symbiotic Mira, using the Stratospheric Observatory for Infrared Astronomy (SOFIA). New photometric and spectroscipic data were obtained with the Faint Object infraRed CAmera for the SOFIA Telescope in 2018 and 2019 after the system had started its "ec…

2022 The Astrophysical Journal
ISO 1