An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``photo-dissociation regions'' (PDRs) and ``X-ray dominated regions'' (XDRs) is presented. Applications of the models are shown to observations of the ultra-luminous infrared galaxy Mrk 231, and the starburst galaxy M 82
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``pho...
An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``pho...
An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``pho...
The radiation from stars and active galactic nuclei (AGN) creates photodissociation regions (PDRs) a...
Photodissociation regions (PDRs) are gas phases in which far-ultraviolet radiation plays a significa...
Photodissociation regions (PDRs) are gas phases in which far-ultraviolet radiation plays a significa...
We present a far-ultraviolet (PDR) and an X-ray dominated region (XDR) code. We include and discuss ...
We present a far-ultraviolet (PDR) and an X-ray dominated region (XDR) code. We include and discuss ...
We present a far-ultraviolet (PDR) and an X-ray dominated region (XDR) code. We include and discuss ...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``pho...
An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``pho...
An overview of the important thermal and chemical processes in ``photon-dominated regions'' or ``pho...
The radiation from stars and active galactic nuclei (AGN) creates photodissociation regions (PDRs) a...
Photodissociation regions (PDRs) are gas phases in which far-ultraviolet radiation plays a significa...
Photodissociation regions (PDRs) are gas phases in which far-ultraviolet radiation plays a significa...
We present a far-ultraviolet (PDR) and an X-ray dominated region (XDR) code. We include and discuss ...
We present a far-ultraviolet (PDR) and an X-ray dominated region (XDR) code. We include and discuss ...
We present a far-ultraviolet (PDR) and an X-ray dominated region (XDR) code. We include and discuss ...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...
Massive stars disrupt their natal molecular cloud material by dissociating molecules, ionizing atoms...