Navigation überspringen
Universitätsbibliothek Heidelberg
Status: Bibliographieeintrag

Verfügbarkeit
Standort: ---
Exemplare: ---
heiBIB
 Online-Ressource
Verfasst von:Wolfire, Mark G. [VerfasserIn]   i
 Vallini, Livia [VerfasserIn]   i
 Chevance, Mélanie [VerfasserIn]   i
Titel:Photodissociation and x-ray-dominated regions
Verf.angabe:Mark G. Wolfire, Livia Vallini and Mélanie Chevance
E-Jahr:2022
Jahr:June 13, 2022
Umfang:73 S.
Fussnoten:Gesehen am 15.09.2022
Titel Quelle:Enthalten in: Annual review of astronomy and astrophysics
Ort Quelle:Palo Alto, Calif. : Annual Reviews Inc., 1963
Jahr Quelle:2022
Band/Heft Quelle:60(2022), Seite 247-318
ISSN Quelle:1545-4282
Abstract: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. PDRs include a wide range of environments, from the diffuse interstellar medium (ISM) to dense star-forming regions. XDRs are found in the center of galaxies hosting AGNs, in protostellar disks, and in the vicinity of X-ray binaries. In this review, we describe the dominant thermal, chemical, and radiation transfer processes in PDRs and XDRs, as well as give a brief description of models and their use for analyzing observations. We then present recent results from Milky Way, nearby extragalactic, and high-redshift observations. Several important results include the following: ▪ Velocity-resolved PDR lines reveal the kinematics of the neutral atomic gas and provide constraints on the stellar feedback process. Their interpretation is, however, in dispute, as observations suggest a prominent role for stellar winds, whereas they are much less important in theoretical models. ▪ A significant fraction of molecular mass resides in CO-dark gas especially in low-metallicity and/or highly irradiated environments. ▪ The CO ladder and [Ci]/[Cii] ratios can determine if FUV or X rays dominate the ISM heating of extragalactic sources. ▪ With Atacama Large Millimeter/submillimeter Array, PDR and XDR tracers are now routinely detected on galactic scales over cosmic time. This makes it possible to link the star-formation history of the Universe to the evolution of the physical and chemical properties of the gas.
DOI:doi:10.1146/annurev-astro-052920-010254
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext: https://doi.org/10.1146/annurev-astro-052920-010254
 DOI: https://doi.org/10.1146/annurev-astro-052920-010254
Datenträger:Online-Ressource
Sprache:eng
Sach-SW:active galactic nuclei
 infrared emission
 interstellar medium
 star-forming regions
K10plus-PPN:181669889X
Verknüpfungen:→ Zeitschrift

Permanenter Link auf diesen Titel (bookmarkfähig):  https://katalog.ub.uni-heidelberg.de/titel/68964491   QR-Code
zum Seitenanfang