Status: Bibliographieeintrag
Standort: ---
Exemplare:
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| Online-Ressource |
Verfasst von: | Wolfire, Mark G. [VerfasserIn]  |
| Vallini, Livia [VerfasserIn]  |
| Chevance, Mélanie [VerfasserIn]  |
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 |
Photodissociation and x-ray-dominated regions / Wolfire, Mark G. [VerfasserIn]; June 13, 2022 (Online-Ressource)
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