Protostars at Subsolar Metallicity: First Detection of Large Solid-state Complex Organic Molecules in the Large Magellanic Cloud
The Astrophysical Journal Letters, vol. 992, pp. L30
Abstract
Abstract We present the results of James Webb Space Telescope observations of the protostar ST6 in the Large Magellanic Cloud (LMC) with the Medium Resolution Spectrograph of the Mid-Infrared Instrument (4.9–27.9 μ m). Characterized by one-third to half-solar metallicity and strong UV radiation fields, the environment of the LMC allows us to study the physics and chemistry of star-forming regions under conditions similar to those at earlier cosmological epochs. We detected five icy complex organic molecules (COMs): methanol (CH 3 OH), acetaldehyde (CH 3 CHO), ethanol (CH 3 CH 2 OH), methyl formate (HCOOCH 3 ), and acetic acid (CH 3 COOH). This is the first conclusive detection of CH 3 COOH ice in an astrophysical context, and CH 3 CHO, CH 3 CH 2 OH, and HCOOCH 3 ices are the first secure detections outside the Galaxy and in a low-metallicity environment. We address the presence of glycolaldehyde (HOCH 2 CHO, a precursor of biomolecules), an isomer of HCOOCH 3 and CH 3 COOH, but its detection is inconclusive. ST6’s spectrum is also rich in simple ices: H 2 O, CO 2 , CH 4 , SO 2 , H 2 CO, HCOOH, OCN − , HCOO − , NH 3 , and NH 4 + . We obtain the composition and molecular abundances in the icy dust mantles by fitting the spectrum in the 6.8–8.4 μ m range with a large sample of laboratory ice spectra using the ENIIGMA fitting tool or the local continuum method. We found differences in the simple and COM ice abundances with respect to H 2 O ice between ST6 and Galactic protostars that likely reflect differences in metallicity and UV flux. More laboratory ice spectra of COMs are needed to better reconstruct the observed infrared spectra of protostars.
Authors 14
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M. Sewiło corresponding
Goddard Space Flight Center · University of Maryland, College Park
Affiliation as printed
Center for Research and Exploration in Space Science and Technology, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Department of Astronomy, University of Maryland, College Park, MD 20742, USA
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Leiden University · Leiden Observatory
Affiliation as printed
Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, NL 2300 RA Leiden, The Netherlands
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Leiden University · Leiden Observatory
Affiliation as printed
Leiden Observatory, Leiden University, PO Box 9513, NL 2300 RA Leiden, The Netherlands
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M. G. Navarro corresponding
Astronomical Observatory of Rome · National Institute for Astrophysics
Affiliation as printed
INAF—Osservatorio Astronomico di Roma, Via di Frascati 33, 00078 Monte Porzio Catone, Italy
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Steven B. Charnley corresponding
Affiliation as printed
Astrochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
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M. Jin corresponding
Goddard Space Flight Center · Catholic University of America
Affiliation as printed
Astrochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Department of Physics, Catholic University of America, Washington, DC 20064, USA
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Joana M. Oliveira corresponding
Affiliation as printed
Lennard-Jones Laboratories, Keele University, ST5 5BG, UK
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Jacco Th. van Loon corresponding
Affiliation as printed
Lennard-Jones Laboratories, Keele University, ST5 5BG, UK
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Leiden University · Leiden Observatory
Affiliation as printed
Leiden Observatory, Leiden University, PO Box 9513, NL 2300 RA Leiden, The Netherlands
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Jennifer J. Wiseman corresponding
Affiliation as printed
Exoplanets and Stellar Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
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R. Indebetouw corresponding
National Radio Astronomy Observatory · University of Virginia
Affiliation as printed
Department of Astronomy, University of Virginia, PO Box 400325, Charlottesville, VA 22904, USA
National Radio Astronomy Observatory, 520 Edgemont Rd., Charlottesville, VA 22903, USA
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C.‐H. Rosie Chen corresponding
Max Planck Institute for Radio Astronomy
Affiliation as printed
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
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Roya Hamedani Golshan corresponding
Affiliation as printed
I. Physikalisches Institut der Universität zu Köln, Zülpicher Str. 77, 50937, Köln, Germany
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D. Qasim corresponding
Affiliation as printed
Southwest Research Institute, 6220 Culebra Rd., San Antonio, TX 78238, USA
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