Photodissociation Region Toolbox

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Ada Coda
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Photodissociation Region Toolbox

Post by Ada Coda » Wed Jul 07, 2021 12:59 pm

Photodissociation Region Toolbox

Abstract: Ultraviolet photons from O and B stars strongly influence the structure and emission spectra of the interstellar medium. The UV photons energetic enough to ionize hydrogen (hν>13.6eV ) will create the H II region around the star, but lower energy UV photons escape. These far-UV photons (6 eV

Credit: Pound, Marc; Wolfire, Mark

Site: https://dustem.astro.umd.edu


Preferred citation method: @INPROCEEDINGS{2008ASPC..394..654P, author = {{Pound}, M.~W. and {Wolfire}, M.~G.}, title = "{The Photo Dissociation Region Toolbox}", booktitle = {Astronomical Data Analysis Software and Systems XVII}, year = 2008, edit

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