The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows

We present James Webb Space Telescope (JWST) Near Infrared Camera observations of the massive star-forming molecular cloud Sagittarius C (Sgr C) in the Central Molecular Zone (CMZ). In conjunction with ancillary mid-IR and far-IR data, we characterize the two most massive protostars in Sgr C via spe...

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Main Authors: Samuel Crowe, Rubén Fedriani, Jonathan C. Tan, Alva Kinman, Yichen Zhang, Morten Andersen, Lucía Bravo Ferres, Francisco Nogueras-Lara, Rainer Schödel, John Bally, Adam Ginsburg, Yu Cheng, Yao-Lun Yang, Sarah Kendrew, Chi-Yan Law, Joseph Armstrong, Zhi-Yun Li
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/ad8889
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author Samuel Crowe
Rubén Fedriani
Jonathan C. Tan
Alva Kinman
Yichen Zhang
Morten Andersen
Lucía Bravo Ferres
Francisco Nogueras-Lara
Rainer Schödel
John Bally
Adam Ginsburg
Yu Cheng
Yao-Lun Yang
Sarah Kendrew
Chi-Yan Law
Joseph Armstrong
Zhi-Yun Li
author_facet Samuel Crowe
Rubén Fedriani
Jonathan C. Tan
Alva Kinman
Yichen Zhang
Morten Andersen
Lucía Bravo Ferres
Francisco Nogueras-Lara
Rainer Schödel
John Bally
Adam Ginsburg
Yu Cheng
Yao-Lun Yang
Sarah Kendrew
Chi-Yan Law
Joseph Armstrong
Zhi-Yun Li
author_sort Samuel Crowe
collection DOAJ
description We present James Webb Space Telescope (JWST) Near Infrared Camera observations of the massive star-forming molecular cloud Sagittarius C (Sgr C) in the Central Molecular Zone (CMZ). In conjunction with ancillary mid-IR and far-IR data, we characterize the two most massive protostars in Sgr C via spectral energy distribution (SED) fitting, estimating that they each have current masses of m _* ∼ 20 M _⊙ and surrounding envelope masses of ∼100 M _⊙ . We report a census of lower-mass protostars in Sgr C via a search for infrared counterparts to millimeter continuum dust cores found with the Atacama Large Millimeter/submillimeter Array (ALMA). We identify 88 molecular hydrogen outflow knot candidates originating from outflows from protostars in Sgr C, the first such unambiguous detections in the infrared in the CMZ. About a quarter of these are associated with flows from the two massive protostars in Sgr C; these extend for over 1 pc and are associated with outflows detected in ALMA SiO line data. An additional ∼40 features likely trace shocks in outflows powered by lower-mass protostars throughout the cloud. We report the discovery of a new star-forming region hosting two prominent bow shocks and several other line-emitting features driven by at least two protostars. We infer that one of these is forming a high-mass star given an SED-derived mass of m _* ∼ 9 M _⊙ and associated massive (∼90 M _⊙ ) millimeter core and water maser. Finally, we identify a population of miscellaneous molecular hydrogen objects that do not appear to be associated with protostellar outflows.
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spelling doaj-art-13dcd16b6d774987b0409bd4930410cc2025-08-20T02:12:55ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-0198311910.3847/1538-4357/ad8889The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar OutflowsSamuel Crowe0https://orcid.org/0009-0005-0394-3754Rubén Fedriani1https://orcid.org/0000-0003-4040-4934Jonathan C. Tan2https://orcid.org/0000-0002-3389-9142Alva Kinman3https://orcid.org/0009-0008-6570-9287Yichen Zhang4https://orcid.org/0000-0001-7511-0034Morten Andersen5https://orcid.org/0000-0002-5306-4089Lucía Bravo Ferres6https://orcid.org/0009-0004-4390-7937Francisco Nogueras-Lara7https://orcid.org/0000-0002-6379-7593Rainer Schödel8https://orcid.org/0000-0001-5404-797XJohn Bally9https://orcid.org/0000-0001-8135-6612Adam Ginsburg10https://orcid.org/0000-0001-6431-9633Yu Cheng11https://orcid.org/0000-0002-8691-4588Yao-Lun Yang12https://orcid.org/0000-0001-8227-2816Sarah Kendrew13https://orcid.org/0000-0002-7612-0469Chi-Yan Law14https://orcid.org/0000-0003-1964-970XJoseph Armstrong15https://orcid.org/0000-0002-4855-1325Zhi-Yun Li16https://orcid.org/0000-0002-7402-6487Department of Astronomy, University of Virginia , Charlottesville, VA 22904, USA ; fec5fg@virginia.eduInstituto de Astrofísica de Andalucía , CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainDepartment of Astronomy, University of Virginia , Charlottesville, VA 22904, USA ; fec5fg@virginia.edu; Department of Space, Earth & Environment, Chalmers University of Technology , 412 93 Gothenburg, SwedenDepartment of Space, Earth & Environment, Chalmers University of Technology , 412 93 Gothenburg, SwedenDepartment of Astronomy, Shanghai Jiao Tong University , 800 Dongchuan Rd., Minhang, Shanghai 200240, People's Republic of ChinaEuropean Southern Observatory , Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, GermanyInstituto de Astrofísica de Andalucía , CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainEuropean Southern Observatory , Karl-Schwarzschild-Strasse 2, D-85748 Garching bei München, GermanyInstituto de Astrofísica de Andalucía , CSIC, Glorieta de la Astronomía s/n, E-18008 Granada, SpainCenter for Astrophysics and Space Astronomy, Astrophysical and Planetary Sciences Department, University of Colorado , UCB 389 Boulder, CO 80309, USADepartment of Astronomy, University of Florida , P.O. Box 112055, Gainesville, FL 32611, USANational Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanStar and Planet Formation Laboratory, RIKEN Cluster for Pioneering Research , Wako, Saitama 351-0198, JapanEuropean Space Agency, Space Telescope Science Institute , Baltimore, MD 21218, USAOsservatorio Astrofisico di Arcetri , Largo Enrico Fermi, 5, 50125 Firenze FI, ItalyDepartment of Space, Earth & Environment, Chalmers University of Technology , 412 93 Gothenburg, SwedenDepartment of Astronomy, University of Virginia , Charlottesville, VA 22904, USA ; fec5fg@virginia.eduWe present James Webb Space Telescope (JWST) Near Infrared Camera observations of the massive star-forming molecular cloud Sagittarius C (Sgr C) in the Central Molecular Zone (CMZ). In conjunction with ancillary mid-IR and far-IR data, we characterize the two most massive protostars in Sgr C via spectral energy distribution (SED) fitting, estimating that they each have current masses of m _* ∼ 20 M _⊙ and surrounding envelope masses of ∼100 M _⊙ . We report a census of lower-mass protostars in Sgr C via a search for infrared counterparts to millimeter continuum dust cores found with the Atacama Large Millimeter/submillimeter Array (ALMA). We identify 88 molecular hydrogen outflow knot candidates originating from outflows from protostars in Sgr C, the first such unambiguous detections in the infrared in the CMZ. About a quarter of these are associated with flows from the two massive protostars in Sgr C; these extend for over 1 pc and are associated with outflows detected in ALMA SiO line data. An additional ∼40 features likely trace shocks in outflows powered by lower-mass protostars throughout the cloud. We report the discovery of a new star-forming region hosting two prominent bow shocks and several other line-emitting features driven by at least two protostars. We infer that one of these is forming a high-mass star given an SED-derived mass of m _* ∼ 9 M _⊙ and associated massive (∼90 M _⊙ ) millimeter core and water maser. Finally, we identify a population of miscellaneous molecular hydrogen objects that do not appear to be associated with protostellar outflows.https://doi.org/10.3847/1538-4357/ad8889Galactic centerMassive starsStellar jetsStar formationH II regionsStellar bow shocks
spellingShingle Samuel Crowe
Rubén Fedriani
Jonathan C. Tan
Alva Kinman
Yichen Zhang
Morten Andersen
Lucía Bravo Ferres
Francisco Nogueras-Lara
Rainer Schödel
John Bally
Adam Ginsburg
Yu Cheng
Yao-Lun Yang
Sarah Kendrew
Chi-Yan Law
Joseph Armstrong
Zhi-Yun Li
The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
The Astrophysical Journal
Galactic center
Massive stars
Stellar jets
Star formation
H II regions
Stellar bow shocks
title The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
title_full The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
title_fullStr The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
title_full_unstemmed The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
title_short The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
title_sort jwst nircam view of sagittarius c i massive star formation and protostellar outflows
topic Galactic center
Massive stars
Stellar jets
Star formation
H II regions
Stellar bow shocks
url https://doi.org/10.3847/1538-4357/ad8889
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