Radio galaxies at TeV energies:
It is common believe that the centers of all galaxies exhibit supermassive black holes with masses ranging from millions up to billions of the mass of our Sun. By accreting surrounding matter, the luminosity of these galactic nuclei can outshine the emission of their host galaxies. If this is the ca...
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Basel ; Beijing ; Wuhan ; Barcelona ; Belgrade
MDPI
[2020]
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| Zusammenfassung: | It is common believe that the centers of all galaxies exhibit supermassive black holes with masses ranging from millions up to billions of the mass of our Sun. By accreting surrounding matter, the luminosity of these galactic nuclei can outshine the emission of their host galaxies. If this is the case, they are called active galactic nuclei. Some of these objects eject powerful outflows composed of plasma, called jets. These jets can produce non-thermal radiation which observable across the entire electromagnetic spectrum from radio up to the gamma-ray frequencies. At highest frequencies (TeV range) most of the detected active galaxies have jets directed along or close to the line of sight. However, also galaxies with larger angles to the line of sight showing fascinating features were discovered, in seeming contradiction to traditional models for these so-called radio galaxies. Thus, the latter are of particular importance for understanding active galactic nuclei in general. This Special Issue contains reviews and research articles about the current knowledge of radio galaxies at TeV energies, including observational results and theoretical models. It is intended to guide the interested reader deeper into this fascinating discipline of modern day astronomy |
| Beschreibung: | Aus dem Impressum: This is a reprint of articles from the Special Issue published online in the open access journal "Galaxies" (ISSN2075-4434) from 2018 to 2020 |
| Beschreibung: | 1 Online-Ressource (vii, 177 Seiten) |
| ISBN: | 9783039287512 |
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| isbn | 9783039287512 |
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| spelling | Radio galaxies at TeV energies special issue editor: Dorit Glawion Basel ; Beijing ; Wuhan ; Barcelona ; Belgrade MDPI [2020] 1 Online-Ressource (vii, 177 Seiten) txt rdacontent c rdamedia cr rdacarrier Aus dem Impressum: This is a reprint of articles from the Special Issue published online in the open access journal "Galaxies" (ISSN2075-4434) from 2018 to 2020 It is common believe that the centers of all galaxies exhibit supermassive black holes with masses ranging from millions up to billions of the mass of our Sun. By accreting surrounding matter, the luminosity of these galactic nuclei can outshine the emission of their host galaxies. If this is the case, they are called active galactic nuclei. Some of these objects eject powerful outflows composed of plasma, called jets. These jets can produce non-thermal radiation which observable across the entire electromagnetic spectrum from radio up to the gamma-ray frequencies. At highest frequencies (TeV range) most of the detected active galaxies have jets directed along or close to the line of sight. However, also galaxies with larger angles to the line of sight showing fascinating features were discovered, in seeming contradiction to traditional models for these so-called radio galaxies. Thus, the latter are of particular importance for understanding active galactic nuclei in general. This Special Issue contains reviews and research articles about the current knowledge of radio galaxies at TeV energies, including observational results and theoretical models. It is intended to guide the interested reader deeper into this fascinating discipline of modern day astronomy Teraelektronenvoltbereich (DE-588)4450797-5 gnd rswk-swf Radiogalaxie (DE-588)4176825-5 gnd rswk-swf Science (General) Physics Astronomy Radiogalaxie (DE-588)4176825-5 s Teraelektronenvoltbereich (DE-588)4450797-5 s DE-604 Glawion, Dorit 1987- (DE-588)1073340465 edt Erscheint auch als Druck-Ausgabe 978-3-03928-750-5 https://www.doabooks.org/doab?func=fulltext&uiLanguage=en&rid=46087 Verlag kostenfrei Volltext |
| spellingShingle | Radio galaxies at TeV energies Teraelektronenvoltbereich (DE-588)4450797-5 gnd Radiogalaxie (DE-588)4176825-5 gnd |
| subject_GND | (DE-588)4450797-5 (DE-588)4176825-5 |
| title | Radio galaxies at TeV energies |
| title_auth | Radio galaxies at TeV energies |
| title_exact_search | Radio galaxies at TeV energies |
| title_exact_search_txtP | Radio galaxies at TeV energies |
| title_full | Radio galaxies at TeV energies special issue editor: Dorit Glawion |
| title_fullStr | Radio galaxies at TeV energies special issue editor: Dorit Glawion |
| title_full_unstemmed | Radio galaxies at TeV energies special issue editor: Dorit Glawion |
| title_short | Radio galaxies at TeV energies |
| title_sort | radio galaxies at tev energies |
| topic | Teraelektronenvoltbereich (DE-588)4450797-5 gnd Radiogalaxie (DE-588)4176825-5 gnd |
| topic_facet | Teraelektronenvoltbereich Radiogalaxie |
| url | https://www.doabooks.org/doab?func=fulltext&uiLanguage=en&rid=46087 |
| work_keys_str_mv | AT glawiondorit radiogalaxiesattevenergies |