English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
 
 
DownloadE-Mail
 Local TagsRelease HistoryDetailsSummary
  Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT

Principe, G., Mitchell, A., Hinton, J., Caroff, S., Parsons, R. D., Hahn, J., et al. (2019). Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT. Proceedings of Science, ICRC2019: 595. Retrieved from http://arxiv.org/abs/1909.11367.

Item is

 

show all hide all

Basic

show hide
Item Permalink: https://hdl.handle.net/21.11116/0000-0005-72AF-6 Version Permalink: https://hdl.handle.net/21.11116/0000-0005-72B0-3
Genre: Conference Paper

Files

show Files
hide Files
:
1909.11367.pdf (Preprint), 961KB
View   Save
File Permalink:
https://hdl.handle.net/21.11116/0000-0005-72B1-2
Name:
1909.11367.pdf
Description:
File downloaded from arXiv at 2020-01-09 10:21
OA-Status:
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
View
Copyright Date:
-
Copyright Info:
-
License:
http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Locators

show

Creators

show
hide
 Creators:
Principe, Giacomo, Author
Mitchell, Alison1, Author           
Hinton, Jim2, Author           
Caroff, Sami, Author
Parsons, Robert Daniel2, Author           
Hahn, Joachim2, Author           
Funk, Stefan, Author
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society, ou_2074298              

Content

show
hide
Free keywords: Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 Abstract: Taking advantage of 10 years of Fermi-LAT data, we perform a new and deep
analysis of the pulsar wind nebula (PWN) HESS J1825-137. We present the results
of the spectral analysis and of the first energy-resolved morphological study
of the PWN HESS J1825-137 from 1 GeV to 1 TeV. This PWN is an archetypal system
making it a perfect laboratory for studying particle transport mechanisms.
Combining this analysis with recent H.E.S.S. results enables a more complete
picture of the nebula to emerge.

Details

show
hide
Language(s):
 Dates: 2019-07
 Publication Status: Published online
 Pages: 7 pages, 6 figures, published in in proceedings of science for the 36th International Cosmic Ray Conference (ICRC2019
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 1909.11367
URI: http://arxiv.org/abs/1909.11367
 Degree: -

Event

show
hide
Title: 36th International Cosmic Ray Conference (ICRC2019)
Place of Event: -
Start-/End Date: -

Legal Case

show

Project information

show

Source 1

show
hide
Title: Proceedings of Science
  Other : PoS
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: ICRC2019 Sequence Number: 595 Start / End Page: - Identifier: ISSN: 1824-8039
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000018850_1