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About:
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
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scientific article published in the Astrophysical Journal
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rdf:type
Item
description
artículu científicu
(ast)
wetenschappelijk artikel
(nl)
наукова стаття, опублікована в серпні 2006
(uk)
im August 2006 veröffentlichter wissenschaftlicher Artikel
(de)
article publié dans la revue scientifique Astrophysical Journal
(fr)
scientific article published in the Astrophysical Journal
(en)
publication date
wds:Q57541877-B93EE60B-5CE4-4601-9D63-82E433AE6179
publication date
2006-08-18 00:00:00Z
(
xsd:dateTime
)
language of work or name
wds:Q57541877-1E1DADCF-5F54-4F81-B35D-DA2C0C616BCD
language of work or name
English
author name string
wds:Q57541877-59BC8C94-5681-4FAF-B0AF-8DED47387784
wds:Q57541877-740D9F81-F959-4859-A81C-55CD9BFE196F
wds:Q57541877-E5F264D3-343E-4340-9043-5FDC81B96965
author name string
Andrew W. Strong
Igor V. Moskalenko
Troy A. Porter
rdfs:label
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(en)
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(nl)
skos:prefLabel
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(en)
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(nl)
name
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(en)
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(nl)
title
wds:Q57541877-14676F50-D652-4B37-9B35-556D1C75FA71
title
Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
(en)
page(s)
wds:Q57541877-3B6A9089-4F5B-40DE-8637-3CB6F98425E3
page(s)
29–32
instance of
wds:Q57541877-DB1E7202-0FB9-47B3-A869-D4290BB8DA45
instance of
scholarly article
published in
wds:Q57541877-9ED4C5F0-DA1F-49B6-95B2-CDD9D3AC42FE
full work available at URL
wds:Q57541877-AEED818F-06C4-496B-A2E6-5F2C1C4ADF24
published in
The Astrophysical Journal
full work available at URL
https://iopscience.iop.org/article/10.1086/507770/pdf
issue
wds:Q57541877-A65B2F2D-178A-470F-ABF6-1E3E5C954AE3
volume
wds:Q57541877-6E67FBC6-B00B-49A5-B767-E529EF029298
issue
1
volume
648
DOI
wds:Q57541877-52F0819C-CB27-405E-B925-ABA9FDE6296A
DOI
http://dx.doi.org/10.1086/507770
DOI
10.1086/507770
arXiv ID
wds:Q57541877-8476A7DA-F248-44C4-BA6E-D4502A1B106A
arXiv ID
astro-ph/0607344
ADS bibcode
wds:Q57541877-1D124B98-C259-4C55-9803-EAE777CD65BE
ADS bibcode
2006ApJ...648L..29P
is
about
of
https://www.wikidata.org/wiki/Special:EntityData/Q57541877
is
cites work
of
A lower limit of 50 microgauss for the magnetic field near the Galactic Centre
Can the Morphology ofγ-Ray Emission Distinguish Annihilating from Decaying Dark Matter?
XMM-Newton observations of HESS J1813-178 reveal a composite Supernova remnant
Discovery of TeVγ-ray emission from the pulsar wind nebula 3C 58 by MAGIC
is
cites work
of
wds:Q56933931-ED6E4F66-E5DE-4D12-AEEC-50439A337263
wds:Q57628454-4393EAC5-9AE1-4330-A85C-68BC57DDF1FC
wds:Q58357445-86E9FC39-FE5A-4A79-A300-39F26F60880F
wds:Q44745048-DAB31B8E-C99A-4942-A725-FCDC1C644468
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