About: Why did Supernova 1054 shine at late times?

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scientific article published in Astronomy and Astrophysics

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в січні 2001 (uk) im Januar 2001 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astronomy and Astrophysics (fr) scientific article published in Astronomy and Astrophysics (en)
publication date	wds:Q56562682-1B2E4AAA-646D-4AA3-B421-0FC3C8932EB0
publication date	2001-01-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q56562682-9D222C87-7D7F-49FF-BA96-00B7D15B5E0D
language of work or name	English
cites work	wds:Q56562682-03E98BF3-1D1B-42F9-8354-59C902469C59 wds:Q56562682-2735BD0C-0AA7-47D5-B25E-2D1F26FA2F0A wds:Q56562682-284A5427-592A-433F-A8A6-6A1D985BFB6D wds:Q56562682-2C0C0761-93A8-4434-AD07-9A53D3289DA6 wds:Q56562682-3594C538-FC3B-4110-BF81-8FC2CDA22176 wds:Q56562682-3EE902BA-2B9D-47EE-8BC3-CFBBA566136D wds:Q56562682-4776D7DC-32CF-4F73-A1FF-0756BC0A26EA wds:Q56562682-504B84B4-5EA6-445F-B5D4-19E676C2C20F wds:Q56562682-506FC27D-EEBD-4197-83F4-90C6CA37DB3A wds:Q56562682-58090F52-70BB-431E-8AC2-99DF9C4B17A5 wds:Q56562682-5E5F006C-E7B7-476B-8CD4-CD1B28EBFACD wds:Q56562682-6D734019-0657-4CC9-A40A-24BD5A16A3A3 wds:Q56562682-750BEA4C-ED5B-4662-95CB-016BBEA0C03B wds:Q56562682-76EAA00B-9859-47AF-AF52-85FED22D0703 wds:Q56562682-7833D30F-CEF5-4E27-9631-CE15DD6E8838 wds:Q56562682-78D219A4-827F-49B4-9068-A35BEA5BA60D wds:Q56562682-7EC4EA69-0083-45AF-BAB5-88A67C78A17E wds:Q56562682-964506EF-3BE7-4CDB-BFD5-640C3DBB2714 wds:Q56562682-9F67A255-0CE9-4693-AA19-431F223A5E6B wds:Q56562682-AD4AFCF9-7712-4FD5-A287-7AB14ED9B869 wds:Q56562682-ADE89B15-AAE0-4078-87F0-4B41587F60AD wds:Q56562682-C97F59F2-AFCA-4F48-A674-252E8AF3A78F wds:Q56562682-CF8BD90E-1116-47EA-8B73-667E6C5247B8 wds:Q56562682-D03FD969-8744-41FB-AB7B-0E8E163CB3C8 wds:Q56562682-EA88A4B0-AB7D-43F2-B1D6-FD67BA4CE4AE wds:Q56562682-EE19AE3B-2BA4-4ACE-B0FD-A6D23424CF5E
cites work	Recent Developments Concerning the Crab Nebula The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis The Peculiar Type II Supernova 1997D: A Case for a Very Low [TSUP]56[/TSUP]N[CLC]i[/CLC] Mass An Optical Study of the Circumstellar Environment Around the Crab Nebula A Reinterpretation of Historical References to the Supernova ofa.d.1054 Radiation Dynamics, Envelope Ejection, and Supernova Light Curves Observations of the Crab Nebula and Its Pulsar in the Far‐Ultraviolet and in the Optical A Very Low Mass of56Ni in the Ejecta of SN 1994W The Crab Nebula's progenitor Optical spectrum of SN 1978K: emission from shocked clouds in the circumstellar wind WFPC2 Studies of the Crab Nebula. II. Ionization Structure of the Crab Filaments The Distance to the Crab Nebula and NP 0532 Three dimensional structure of the Crab nebula Type I supernovae, R Coronae Borealis stars, and the Crab nebula XX. Elemental abundances in the Crab nebula The bolometric light curve of SN 1987A. I. Results from ESO and CTIO U and Q0 photometry Late spectral evolution of SN 1987A. I. Temperature and ionization The unusual nickel/iron abundance ratio in the Crab nebula filaments Pulsar nebulae in supernovae Emission from circumstellar interaction in normal type II supernovae Excitation of [Ni II] and [Fe II] lines in gaseous nebulae Neutron star accretion in a supernova Modeling the evolution of disk galaxies. II. Yields of massive stars The energy source powering the late-time bolometric evolution of SN 1987A Gamma-ray deposition and nonthermal excitation in supernovae Late spectral evolution of SN 1987A. II. Line emission
author name string	wds:Q56562682-05EA6080-4821-42DC-B897-F962B453ED32
author name string	C. Kozma
rdfs:label	Why did Supernova 1054 shine at late times? (en) Why did Supernova 1054 shine at late times? (nl)
skos:prefLabel	Why did Supernova 1054 shine at late times? (en) Why did Supernova 1054 shine at late times? (nl)
name	Why did Supernova 1054 shine at late times? (en) Why did Supernova 1054 shine at late times? (nl)
author	wds:Q56562682-0277090F-1B9D-4475-AB5F-B92CFFC1D67B wds:Q56562682-03E17D4A-5DB9-4388-B642-40857F4E2AED
author	Jesper Sollerman Peter Lundqvist
title	wds:Q56562682-37BDEF2F-3DC2-4947-9A2E-E709C729E6D7
title	Why did Supernova 1054 shine at late times? (en)
page(s)	wds:Q56562682-699F969D-932F-4A44-BB3C-E076A6208698
page(s)	197–201
instance of	wds:Q56562682-1F169B49-5084-44F2-8430-D86773ED757D
instance of	scholarly article
published in	wds:Q56562682-65399AE2-F014-4F02-9AB9-DF45686887D6
published in	Astronomy and Astrophysics
issue	wds:Q56562682-1A8B6C79-D1BA-425E-A3C6-27FAFD62A6DC
volume	wds:Q56562682-5E92F622-5657-4EDC-AB83-4C8CB192AD87
issue	1
volume	366
DOI	wds:Q56562682-CE088CFE-B7C0-440F-A7EC-386D9D4CCE30
DOI	http://dx.doi.org/10.1051/0004-6361:20000211
DOI	10.1051/0004-6361:20000211
ResearchGate publication ID	wds:Q56562682-C6B51FAB-70D6-4C38-AE2C-2852ED2FA812
ResearchGate publication ID	2227061
arXiv ID	wds:Q56562682-240ACAD0-554F-46D9-86EE-B6EE9AB7D542
arXiv ID	astro-ph/0012347
ADS bibcode	wds:Q56562682-9B528772-35B6-4BE1-AC2F-2425421FC876
ADS bibcode	2001A&A...366..197S
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56562682
is cites work of	Optical and infrared observations of the Crab Pulsar and its nearby knot Observational and theoretical constraints for an Hα-halo around the Crab nebula The Crab pulsar and its red knot in the near-infrared

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