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JWST/MIRI Spectroscopy of the Disk of the Young Eruptive Star EX Lup in Quiescence
DOI: 10.3847/2041-8213/acb58a Bibcode: 2023ApJ...945L...7K

Banzatti, Andrea; Henning, Thomas; Bouwman, Jeroen +7 more

EX Lup is a low-mass pre-main-sequence star that occasionally shows accretion-related outbursts. Here, we present JWST/MIRI medium-resolution spectroscopy obtained for EX Lup 14 yr after its powerful outburst. EX Lup is now in quiescence and displays a Class II spectrum. We detect a forest of emission lines from molecules previously identified in …

2023 The Astrophysical Journal
ISO JWST 38
JWST: Deuterated PAHs, PAH Nitriles, and PAH Overtone and Combination Bands. I. Program Description and First Look
DOI: 10.3847/1538-4357/ad022b Bibcode: 2023ApJ...959...74B

Boersma, C.; Bregman, J. D.; Allamandola, L. J. +6 more

A first look is taken at the NIRSpec 1-5 µm observations from James Webb Space Telescope program 1591 that targets seven objects along the low-mass stellar life cycle with polycyclic aromatic hydrocarbon (PAH) emission. Spectra extracted from a 1.″5 radius circular aperture are explored, showing a wealth of features, including the 3 µm…

2023 The Astrophysical Journal
ISO eHST JWST 22
Dissecting the Mid-infrared Heart of M83 with JWST
DOI: 10.3847/1538-4357/acc837 Bibcode: 2023ApJ...948..124H

Kumari, Nimisha; Hirschauer, Alec S.; Hernandez, Svea +10 more

We present a first look at the MRS observations of the nucleus of the nearby galaxy M83, taken with MIRI on board JWST. The observations show a rich set of emission features from the ionized gas, warm molecular gas, and dust. To begin dissecting the complex processes in this part of the galaxy, we divide the observations into four different region…

2023 The Astrophysical Journal
ISO eHST JWST 10
The Mid-infrared Molecular Inventory toward Orion IRc2
DOI: 10.3847/1538-4357/aca6e8 Bibcode: 2023ApJ...945...26N

Drozdovskaya, Maria N.; Herbst, Eric; Acharyya, Kinsuk +8 more

We present the first high spectral resolution mid-infrared survey in the Orion BN/KL region, covering 7.2–28.3 µm. With SOFIA/EXES, we target the enigmatic source Orion IRc2. While this is in the most prolifically studied massive star-forming region, longer wavelengths and molecular emission lines dominated previous spectral surveys. The mid…

2023 The Astrophysical Journal
ISO 10
Halfway to the Peak: Spatially Resolved Star Formation and Kinematics in a z = 0.54 Dusty Galaxy with JWST/MIRI
DOI: 10.3847/2041-8213/ad07e1 Bibcode: 2023ApJ...958L...5Y

Veilleux, Sylvain; Ogle, Patrick; Alberts, Stacey +16 more

We present JWST Mid-InfraRed Instrument/Medium-Resolution Spectrometer (MIRI/MRS) observations of an infrared luminous disk galaxy, FLS1, at z ~ 0.54. With a lookback time of 5 Gyr, FLS1 is chronologically at the midpoint between the peak epoch of star formation and the present day. The MRS data provide maps of the atomic fine structure lines [Ar …

2023 The Astrophysical Journal
ISO eHST JWST 5
Raman Scattering by Atomic Hydrogen in Photodissociation Regions: An Alternative to the Polycyclic Aromatic Hydrocarbons Hypothesis
DOI: 10.3847/1538-4357/acdad0 Bibcode: 2023ApJ...952..116Z

Zagury, Frédéric

Photodissociation regions (PDRs) illuminated by high temperature (T > 104 K) radiation fields display characteristic optical to midinfrared spectral features: emission bands that cluster around the blue limits of hydrogen series, an extended red emission (ERE) in the vicinity of Hα, and a continuum in the infrared part of the spectru…

2023 The Astrophysical Journal
ISO 3
High-resolution SOFIA/EXES Spectroscopy of Water Absorption Lines in the Massive Young Binary W3 IRS 5
DOI: 10.3847/1538-4357/ace16e Bibcode: 2023ApJ...953..103L

Montiel, Edward; Neufeld, David; Indriolo, Nick +9 more

We present in this paper mid-infrared (5-8 µm) spectroscopy toward the massive young binary W3 IRS 5, using the Echelon Cross Echelle Spectrograph (EXES) spectrometer in high-resolution mode (R ~ 50,000) from the NASA Stratospheric Observatory for Infrared Astronomy (SOFIA). Many (~180) ν 2 = 1-0 and (~90) ν 2 = 2-1 abs…

2023 The Astrophysical Journal
ISO 3