JWST-IPA: Chemical Inventory and Spatial Mapping of Ices in the Protostar HOPS 370—Evidence for an Opacity Hole and Thermal Processing of Ices

Abstract The composition of protoplanetary disks, and hence the initial conditions of planet formation, may be strongly influenced by the infall and thermal processing of material during the protostellar phase. The composition of dust and ice in protostellar envelopes, shaped by energetic processes driven by the protostar, serves as the fundamental building material for planets and complex organic molecules. As part of the JWST General Observers program, “Investigating Protostellar Accretion,” we observed an intermediate-mass protostar HOPS 370 (OMC2-FIR3) using NIRSpec integral field unit and Mid-Infrared Instrument medium-resolution spectroscopy. This study presents the gas and ice phase chemical inventory revealed with the JWST in the spectral range of ∼2.9–28 μ m and explores the spatial variation of volatile ice species in the protostellar envelope. We find evidence for the thermal processing of ice species throughout the inner envelope. We present the first high-spatial resolution (∼80 au) maps of key volatile ice species H 2 O, CO 2 , 13 CO 2 , CO, and OCN − , which reveal a highly structured and inhomogeneous density distribution of the protostellar envelope, with a deficiency of ice column density that coincides with the jet/outflow shocked knots. Further, we observe high relative crystallinity of H 2 O ice around the shocked knot seen in the H 2 and OH wind/outflow, which can be explained by a lack of outer colder material in the envelope along the line of sight due to the irregular structure of the envelope. These observations show clear evidence of thermal processing of the ices in the inner envelope, close to the outflow cavity walls, heated by the luminous protostar.

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Journal
The Astrophysical Journal
Published
2025-04-11
DOI
https://doi.org/10.3847/1538-4357/adb71f
Citations
8
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
9.24

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article

JWST-IPA: Chemical Inventory and Spatial Mapping of Ices in the Protostar HOPS 370—Evidence for an Opacity Hole and Thermal Processing of Ices

Pooneh Nazari, John Tobin, Joel D. Green, Robert Gutermuth et al.
8 citations
The Astrophysical Journal
Astrophysics and Star Formation Studies
9.24
article

JWST-IPA: Chemical Inventory and Spatial Mapping of Ices in the Protostar HOPS 370—Evidence for an Opacity Hole and Thermal Processing of Ices

Pooneh Nazari, John Tobin, Joel D. Green, Robert Gutermuth, Samuel Federman, Wafa Zakri, P. Manoj, S. J. Wolk, A. Caratti o Garatti, Nolan Habel, H. Linz, Łukasz Tychoniec, Nashanty G. C. Brunken, Tyler L. Bourke, Prabhani Atnagulov, Thomas Stanke, S. T. Megeath, Pamela Klaassen, Yao-Lun Yang, James Muzerolle Page, William J. Fischer, Mayank Narang, Adam E. Rubinstein, E. F. van Dishoeck, Leslie W. Looney, David A. Neufeld, D. M. Watson, H. Beuther, Elise Furlan, Rohan Rahatgaonkar, W. R. M. Rocha, Guillem Anglada, Amelia M. Stutz, Nicole Karnath, K. Slavicinska, Neal J. Evans, Patrick Sheehan, Mayra Osorio, Himanshu Tyagi
article en
8 citations

Abstract

Abstract The composition of protoplanetary disks, and hence the initial conditions of planet formation, may be strongly influenced by the infall and thermal processing of material during the protostellar phase. The composition of dust and ice in protostellar envelopes, shaped by energetic processes driven by the protostar, serves as the fundamental building material for planets and complex organic molecules. As part of the JWST General Observers program, “Investigating Protostellar Accretion,” we observed an intermediate-mass protostar HOPS 370 (OMC2-FIR3) using NIRSpec integral field unit and Mid-Infrared Instrument medium-resolution spectroscopy. This study presents the gas and ice phase chemical inventory revealed with the JWST in the spectral range of ∼2.9–28 μ m and explores the spatial variation of volatile ice species in the protostellar envelope. We find evidence for the thermal processing of ice species throughout the inner envelope. We present the first high-spatial resolution (∼80 au) maps of key volatile ice species H 2 O, CO 2 , 13 CO 2 , CO, and OCN − , which reveal a highly structured and inhomogeneous density distribution of the protostellar envelope, with a deficiency of ice column density that coincides with the jet/outflow shocked knots. Further, we observe high relative crystallinity of H 2 O ice around the shocked knot seen in the H 2 and OH wind/outflow, which can be explained by a lack of outer colder material in the envelope along the line of sight due to the irregular structure of the envelope. These observations show clear evidence of thermal processing of the ices in the inner envelope, close to the outflow cavity walls, heated by the luminous protostar.

The Astrophysical JournalVol. 983(2)
Tata Institute of Fundamental Research (IN), Leiden University (NL), California Institute of Technology (US), Space Telescope Science Institute (US), Space Science Institute (US), Institute of Astronomy and Astrophysics, Academia Sinica (TW), European Southern Observatory (DE), Jet Propulsion Laboratory (US), Johns Hopkins University (US), University of Illinois Urbana-Champaign (US), University of Concepción (CL), University of Massachusetts Amherst (US), National Radio Astronomy Observatory (US), Astronomical Observatory of Capodimonte (IT), Max Planck Institute for Extraterrestrial Physics (DE), SKA Observatory (GB), Max Planck Institute for Astronomy (DE), RIKEN (JP), Université Bourgogne Franche-Comté (FR), Gemini South Observatory (CL), Center for Astrophysics Harvard & Smithsonian (US), Instituto de Astrofísica de Andalucía (ES), Infrared Processing and Analysis Center (US), UK Astronomy Technology Centre (GB), University of Rochester (US), University of Baltimore (US), Friedrich Schiller University Jena (DE), The University of Texas at Austin (US), University of Toledo (US), Jazan University (SA)
National Aeronautics and Space Administration, Gruber Foundation, Space Telescope Science Institute, Universities Space Research Association, European Commission, Department of Atomic Energy, Government of India, Agencia Nacional de Investigación y Desarrollo, RIKEN, Agencia Estatal de Investigación
Openalex Percentile: Top 2%
Astrophysics and Star Formation Studies
9.24
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