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Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
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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 2003
(uk)
im August 2003 veröffentlichter wissenschaftlicher Artikel
(de)
article publié dans la revue scientifique Astrophysical Journal
(fr)
scientific article published in the Astrophysical Journal
(en)
publication date
wds:Q58249114-DE836BAB-51DA-4BA4-9B9A-4AA777539FAA
publication date
2003-08-10 00:00:00Z
(
xsd:dateTime
)
language of work or name
wds:Q58249114-E40F8E7C-1265-429D-AAE7-B88485AF8249
language of work or name
English
author name string
wds:Q58249114-54FF1C4A-9129-438A-877D-2A8D44A375AF
wds:Q58249114-6D752E3A-2599-4C64-81FA-7D7EAB28932F
author name string
Kazimierz J. Borkowski
Inmaculada Dominguez
rdfs:label
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(en)
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(nl)
skos:prefLabel
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(en)
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(nl)
name
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(en)
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(nl)
author
wds:Q58249114-4B0D9105-0AB9-4F15-86CC-B9A197AD53A4
wds:Q58249114-8A74F7E7-6E75-4567-8793-F685555DBB52
author
Eduardo Bravo
Carles Badenes
title
wds:Q58249114-D8F939BB-B228-4F6D-861C-5D8A21C4DAA8
title
Thermal X‐Ray Emission from Shocked Ejecta in Type Ia Supernova Remnants: Prospects for Explosion Mechanism Identification
(en)
page(s)
wds:Q58249114-56D9D49C-A053-44B8-B418-AEF92EE36666
page(s)
358–369
instance of
wds:Q58249114-A1F87050-84B7-4C17-8280-FA1093E9BB21
instance of
scholarly article
published in
wds:Q58249114-37F962CC-910C-4613-97EA-F1E769A172F8
full work available at URL
wds:Q58249114-99EAC837-6AF5-445A-844C-C101B09FDFF4
published in
The Astrophysical Journal
full work available at URL
https://iopscience.iop.org/article/10.1086/376448/pdf
issue
wds:Q58249114-2121947D-011C-498D-A76B-E4D9B6A9FA22
volume
wds:Q58249114-83A397C3-5AEB-4C6A-8E38-E206314FA0FB
issue
1
volume
593
DOI
wds:Q58249114-FD65D215-175E-4A4A-A6F2-281E27635774
DOI
http://dx.doi.org/10.1086/376448
DOI
10.1086/376448
arXiv ID
wds:Q58249114-6DE4AE30-5488-4E44-9022-0FEBC8F167BE
arXiv ID
astro-ph/0304552
ADS bibcode
wds:Q58249114-58B65602-F091-4C1C-9E7A-35DAE46FDC58
ADS bibcode
2003ApJ...593..358B
is
about
of
https://www.wikidata.org/wiki/Special:EntityData/Q58249114
is
cites work
of
X-ray studies of supernova remnants: a different view of supernova explosions
Cobalt-56 γ-ray emission lines from the type Ia supernova 2014J.
Supernova Remnants as Clues to Their Progenitors
Observation of SN2011fe with INTEGRAL
The metal contents of two groups of galaxies
Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models
Two evolved supernova remnants with newly identified Fe-rich cores in the Large Magellanic Cloud
Are ^44^Ti-producing supernovae exceptional?
CHEERS: The chemical evolution RGS sample
is
cites work
of
wds:Q58248853-C0A95FA9-E01D-44E6-91FD-9F2AB1E769AD
wds:Q58907422-0C5E990D-7EE3-42C1-8AEC-85053121D6D6
wds:Q57518808-B41C1C85-56F7-401E-BACE-680230B80FDF
wds:Q33842123-CA7C9D49-FE54-40E6-8CE1-1482F1638ED2
wds:Q58907456-C05A10A1-5751-4757-AD02-9B005B16E9D6
wds:Q68592417-2FAA251F-09A0-4E85-AB61-C1A14823E42C
wds:Q58248940-47C6BBCE-C1AE-40E5-844A-9969B21007CA
wds:Q58907412-26A3F881-2E10-499A-92D1-3B5EC4A88A00
wds:Q34435553-6F0DDF1B-1254-4D69-8E3B-E5C766883992
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