Search Publications

Detection of PAH Absorption and Determination of the Mid-infrared Diffuse Interstellar Extinction Curve from the Sight Line toward Cyg OB2-12
DOI: 10.3847/1538-4357/ab8cc3 Bibcode: 2020ApJ...895...38H

Draine, B. T.; Hensley, Brandon S.

The sight line toward the luminous blue hypergiant Cyg OB2-12 is widely used to study interstellar dust on account of its large extinction (AV ≃ 10 mag) and the fact that this extinction appears to be dominated by dust typical of the diffuse interstellar medium. We present a new analysis of archival Infrared Space Observatory Short Wave…

2020 The Astrophysical Journal
Gaia ISO 46
Revisiting the Impact of Dust Production from Carbon-rich Wolf-Rayet Binaries
DOI: 10.3847/1538-4357/ab9cb5 Bibcode: 2020ApJ...898...74L

Sakon, Itsuki; Williams, Peredur M.; Lau, Ryan M. +3 more

We present a dust spectral energy distribution (SED) and binary stellar population analysis revisiting the dust production rates (DPRs) in the winds of carbon-rich Wolf-Rayet (WC) binaries and their impact on galactic dust budgets. DustEM SED models of 19 Galactic WC "dustars" reveal DPRs of ${\dot{M}}_{d}\sim {10}^{-10}\mbox{--}{10}^{-6}$ M⊙…

2020 The Astrophysical Journal
Gaia ISO 33
Surveying the Giant H II Regions of the Milky Way with SOFIA. II. M17
DOI: 10.3847/1538-4357/ab5fd0 Bibcode: 2020ApJ...888...98L

Lim, Wanggi; De Buizer, James M.; Radomski, James T.

We present our second set of results from our mid-infrared imaging survey of Milky Way giant H II regions. We used the FORCAST instrument on the Stratospheric Observatory For Infrared Astronomy (SOFIA) to obtain 20 and 37 µm images of the central ∼10' × 10' area of M17. We investigate the small- and large-scale properties of M17 using our da…

2020 The Astrophysical Journal
Herschel ISO 18
Resolving Decades of Periodic Spirals from the Wolf-Rayet Dust Factory WR 112
DOI: 10.3847/1538-4357/abaab8 Bibcode: 2020ApJ...900..190L

Moffat, Anthony F. J.; Stevens, Ian R.; Sakon, Itsuki +9 more

WR 112 is a dust-forming carbon-rich Wolf-Rayet (WC) binary with a dusty circumstellar nebula that exhibits a complex asymmetric morphology, which traces the orbital motion and dust formation in the colliding winds of the central binary. Unraveling the complicated circumstellar dust emission around WR 112 therefore provides an opportunity to under…

2020 The Astrophysical Journal
ISO 16
The Isotropic Interplanetary Dust Cloud and Near-infrared Extragalactic Background Light Observed with COBE/DIRBE
DOI: 10.3847/1538-4357/abad3d Bibcode: 2020ApJ...901..112S

Matsuura, S.; Sano, K.; Yomo, K. +1 more

We report observation of isotropic interplanetary dust (IPD) by analyzing the infrared (IR) maps of the Diffuse Infrared Background Experiment (DIRBE) on board the Cosmic Background Explorer (COBE) spacecraft. To search for the isotropic IPD, we perform new analysis in terms of the solar elongation angle (ɛ), because we expect the zodiacal light (…

2020 The Astrophysical Journal
AKARI ISO 15
SOFIA-EXES Observations of Betelgeuse during the Great Dimming of 2019/2020
DOI: 10.3847/2041-8213/ab84e6 Bibcode: 2020ApJ...893L..23H

Harper, Graham M.; Guinan, Edward F.; Ryde, Nils +5 more

In 2019 October Betelgeuse began a decline in V-band brightness that went beyond the minimum expected from its quasi-periodic ∼420 day cycle, becoming the faintest in recorded photometric history. Observations obtained in 2019 December with Very Large Telescope/SPHERE have shown that the southern half of the star has become markedly fainter than i…

2020 The Astrophysical Journal
ISO 11
SOFIA/FORCAST Observations of R Aqr: Monitoring the Dust Emission
DOI: 10.3847/1538-4357/ab9824 Bibcode: 2020ApJ...898...31O

Gorti, Uma; Wagner, R. Mark; Sankrit, Ravi +2 more

We present mid-infrared spectra of the symbiotic Mira, R Aqr obtained with the Faint Object infraRed CAmera instrument on the Stratospheric Observatory for Infrared Astronomy in 2016 and 2017. These data, supplemented with Infrared Space Observatory observations from 20 yr earlier, allow us to study the variation of the silicate dust emission over…

2020 The Astrophysical Journal
ISO 2