Radiative Feedback from Massive Stars as Traced by Multiband Imaging and Spectroscopic Mosaics
Stellar Physics
PI: Olivier N. Berne
Co-PIs: Emilie Habart and Els Peeters
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Program Details
Circumstellar Matter
Dust
HII Regions
Interstellar Medium
Molecular CloudsAlain Abergel
Edwin Anthony Bergin
Jeronimo Bernard-Salas
Emeric Bron
Jan Cami
Stephanie Cazaux
Emmanuel Dartois
Asuncion Fuente
Javier Goicoechea
Karl D. Gordon
Yoko Okada
Takashi Onaka
Massimo Robberto
Markus Roellig
Alexander G. G. M. Tielens
Silvia Vicente
Mark WolfireMassive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms and molecules, and heating the gas and dust. These processes drive the evolution of interstellar matter in our Galaxy and throughout the Universe from the era of vigorous star formation at redshifts of 1-3, to the present day. Much of this interaction occurs in Photo-Dissociation Regions (PDRs) where far-ultraviolet photons of these stars create a largely neutral, but warm region of gas and dust. PDR emission dominates the IR spectra of star-forming galaxies and also provides a unique tool to study in detail the physical and chemical processes that are relevant for most of the mass in inter- and circumstellar media including diffuse clouds, protoplanetary disk -and molecular cloud surfaces, globules, planetary nebulae, and starburst galaxies.
We propose to provide template datasets designed to identify key PDR characteristics in JWST spectra in order to guide the preparation of Cycle 2 proposals on star-forming regions in our Galaxy and beyond. We plan to obtain the first spatially resolved, high spectral resolution IR observations of a PDR using NIRCam, NIRSpec and MIRI. These data will test widely used theoretical models and extend them into the JWST era.
MIRI: Medium Resolution Spectroscopy; Imaging
NIRCAM: Imaging
NIRSPEC: IFU Spectroscopy- Maps of spectral features
- Template spectra
- Spectral order stitching and stitched cubes
- Images/spectra cross-calibration
- pyPAHFIT+ (tool to decompose the spectra into PAH bands, gas lines and dust continuum components)
- Line catalog (HII region, Ionization Front, Dissociation Front, molecular zone)
- H2 fitting tool (tool for analysis of H2 lines)
- PDR model toolbox (tool to derive the physical conditions)
- PAHdb spectral analysis tool (decomposition of Polycyclic Aromatic Hydrocarbon or PAH emission)
- Ionized gas lines toolbox
- Telecons open to the community will be organized on a regular basis
- Community workshop
- People interested are welcome to register on our website to keep posted and participate
- JWebbinar 15 - PDRs4all - Simulate NIRCam Observations of an Extended Source. The associated materials and videos can be found on the JWebbinars page.
- JWebbinar 23 - PDRs4ALL: Community Telecons in Support of JWST Cycle 2 Proposals. The associated materials and videos can be found on the JWebbinars page.
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The NASA James Webb Space Telescope, developed in partnership with ESA and CSA, is operated by AURA’s Space Telescope Science Institute.