Results 1 to 10 of about 1,980 (156)
Photodissociation and X-Ray-Dominated Regions
The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions (PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated by far-ultraviolet (FUV) radiation or X-ray radiation, respectively.
Mark Wolfire +2 more
exaly +3 more sources
The Resolved Structure of a Low-metallicity Photodissociation Region
Photodissociation regions (PDRs) are key to understanding the feedback processes that shape interstellar matter in galaxies. One important type of PDR is the interface between H ii regions and molecular clouds, where far-ultraviolet radiation from ...
Ilyse Y. Clark +16 more
doaj +5 more sources
Photoevaporation of Clumps in Photodissociation Regions [PDF]
To appear in the Astrophysical ...
Gorti, Uma, Hollenbach, David
exaly +3 more sources
Wavelength-dependent photofragmentation of pyrazine [PDF]
Ultraviolet (UV) photon-induced dissociation of larger molecules is a rich source of smaller hydrocarbons and nitrogen-bearing molecules in the interstellar medium.
Siddhartha S. Payra +3 more
doaj +2 more sources
Photodissociation regions. I - Basic model. II - A model for the Orion photodissociation region
A theoretical parameter study of the temperature and chemical structure of dense photodissociation regions and their resultant spectrum is presented. Models are discussed which are relevant not only to the dust and gas between molecular clouds and H II regions, but also apply to any neutral cloud illuminated by intense FUV fluxes.
A. G. G. M. Tielens, D. Hollenbach
exaly +2 more sources
Photodissociation regions in the interstellar medium of galaxies [PDF]
The interstellar medium of galaxies is the reservoir out of which stars are born and into which stars inject newly created elements as they age. The physical properties of the interstellar medium are governed in part by the radiation emitted by these stars.
Hollenbach, DJ, Tielens, A G G M
exaly +4 more sources
Low-density photodissociation regions
A theoretical parameter study of the temperature and chemical structure of photodissociation regions (PDRs) and their resultant spectrum is presented. The models, which solve for the chemical and thermal steady state of a one-dimensional slab exposed to an incident FUV flux, relate the observed line and continuum emission from these regions to physical
David J. Hollenbach +2 more
exaly +2 more sources
High-resolution Observations of H i in the IC 63 Reflection Nebula
Photodissociation regions (PDRs), where the (far-)ultraviolet light from hot young stars interact with the gas in surrounding molecular clouds, provide laboratories for understanding the nature and role of feedback by star formation on the interstellar ...
Lars Bonne +9 more
doaj +1 more source
C60IN PHOTODISSOCIATION REGIONS [PDF]
Recent studies have confirmed the presence of buckminsterfullerene (C$_{60}$) in different interstellar and circumstellar environments. However, several aspects regarding C$_{60}$ in space are not well understood yet, such as the formation and excitation processes, and the connection between C$_{60}$ and other carbonaceous compounds in the interstellar
Castellanos +5 more
openaire +2 more sources
SOFIA FEEDBACK Survey: The Pillars of Creation in [C ii] and Molecular Lines
We investigate the physical structure and conditions of photodissociation regions (PDRs) and molecular gas within the Pillars of Creation in the Eagle Nebula using SOFIA FEEDBACK observations of the [C ii ] 158 μ m line.
Ramsey L. Karim +13 more
doaj +1 more source

