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Title:The Cherenkov Telescope Array view of the Galactic Center region
Authors:ID Viana, Aion (Author)
ID Eckner, Christopher (Author)
ID Kukec Mezek, Gašper (Author)
ID Stanič, Samo (Author)
ID Vorobiov, Serguei (Author)
ID Yang, Lili (Author)
ID Zaharijas, Gabrijela (Author)
ID Zavrtanik, Danilo (Author)
ID Zavrtanik, Marko (Author)
ID Zehrer, Lukas (Author), et al.
Files:.pdf ICRC2019_817.pdf (2,78 MB)
MD5: DCF993B75B900BD76BCBA70F27B2C555
 
URL https://pos.sissa.it/358/817/pdf
 
URL https://pos.sissa.it/358/
 
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Language:English
Work type:Unknown
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:Among all the high-energy environments of our Galaxy, the Galactic Center (GC) region is definitely the richest. It harbors a large amount of non-thermal emitters, including the closest supermassive black hole, dense molecular clouds, regions with strong star forming activity, multiple supernova remnants and pulsar wind nebulae, arc-like radio structures, as well as the base of what may be large-scale Galactic outflows, possibly related to the Fermi Bubbles. It also contains a strong diffuse TeV gamma-ray emission along the Galactic ridge, with a disputed origin, including the presence of a possible Pevatron, unresolved sources, and an increased relevance of the diffuse sea of cosmic rays. This very rich region will be one of the key targets for the next generation ground-based observatory for gamma-ray astronomy, the Cherenkov Telescope Array (CTA). Here we review the CTA science case for the study of the GC region, and present the planned survey strategy. These observations are simulated and we assess CTA’s potential to better characterize the origin and nature of a selection of gamma-ray sources in the region.
Keywords:Galactic Center (GC) region, the Cherenkov Telescope Array (CTA) Observatory, supermassive black hole, molecular clouds, star forming regions
Publication status:Published
Publication version:Version of Record
Publication date:01.01.2019
Year of publishing:2019
Number of pages:9 str.
COBISS.SI-ID:214724355 New window
UDC:539.1
ISSN on article:1824-8039
DOI:10.22323/1.358.0817 New window
NUK URN:URN:SI:UNG:REP:NMQQYRHQ
Publication date in RUNG:12.11.2024
Views:62
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Record is a part of a proceedings

Title:36th International Cosmic Ray Conference [also] ICRC2019, Madison, WI, U. S. A., July 24th-August 1st, 2019
COBISS.SI-ID:5444091 New window

Record is a part of a journal

Title:Proceedings of science
Shortened title:Pos proc. sci.
Publisher:Sissa
ISSN:1824-8039
COBISS.SI-ID:20239655 New window

Document is financed by a project

Funder:ARIS - Slovenian Research and Innovation Agency
Funding programme:Raziskovalni program
Project number:P1-0031
Name:Večglasniška astrofizika

Licences

License:CC BY-NC-ND 4.0, Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
Link:http://creativecommons.org/licenses/by-nc-nd/4.0/
Description:The most restrictive Creative Commons license. This only allows people to download and share the work for no commercial gain and for no other purposes.

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