Study of Supernovae Important for Cosmology
The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense s...
Gespeichert in:
Veröffentlicht in: | arXiv.org 2015-02 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Baklanov, P V Blinnikov, S I M Sh Potashov Dolgov, A D |
description | The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense shell method is based on the radiation hydrodynamic model of a supernova. The method of the blackbody model, as well as the correctness of its application for simple estimates of distances from observation data, has been justified. |
doi_str_mv | 10.48550/arxiv.1502.06798 |
format | Article |
fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1502_06798</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2081193673</sourcerecordid><originalsourceid>FETCH-LOGICAL-a523-d6ba3adf53b9e07e2045ea148fac921f3792a592de5a382d363a3545e67916923</originalsourceid><addsrcrecordid>eNotj81Kw0AURgdBsNQ-gCsDLiV15t7cycxSgj-Fgot2H27NjLQ0mThJinl7Y-vq2xw-zhHiTsllZojkE8ef_WmpSMJS6tyaKzEDRJWaDOBGLLruIKUEnQMRzsTjph-qMQk-2Qyti004sUtWdRtiz02f-BCTInR1OIav8VZcez52bvG_c7F9fdkW7-n6421VPK9TJsC00jtGrjzhzjqZO5AZOVaZ8fxpQXnMLTBZqBwxGqhQIyNNzCSrtAWci_vL7bmkbOO-5jiWf0XluWgiHi5EG8P34Lq-PIQhNpNTCdIoZVHniL8U7ky5</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2081193673</pqid></control><display><type>article</type><title>Study of Supernovae Important for Cosmology</title><source>Freely Accessible Journals</source><source>arXiv.org</source><creator>Baklanov, P V ; Blinnikov, S I ; M Sh Potashov ; Dolgov, A D</creator><creatorcontrib>Baklanov, P V ; Blinnikov, S I ; M Sh Potashov ; Dolgov, A D</creatorcontrib><description>The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense shell method is based on the radiation hydrodynamic model of a supernova. The method of the blackbody model, as well as the correctness of its application for simple estimates of distances from observation data, has been justified.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1502.06798</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Blackbody ; Cosmology ; Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - High Energy Physics - Phenomenology ; Supernovae</subject><ispartof>arXiv.org, 2015-02</ispartof><rights>2015. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.1134/S0021364013200034$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.1502.06798$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Baklanov, P V</creatorcontrib><creatorcontrib>Blinnikov, S I</creatorcontrib><creatorcontrib>M Sh Potashov</creatorcontrib><creatorcontrib>Dolgov, A D</creatorcontrib><title>Study of Supernovae Important for Cosmology</title><title>arXiv.org</title><description>The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense shell method is based on the radiation hydrodynamic model of a supernova. The method of the blackbody model, as well as the correctness of its application for simple estimates of distances from observation data, has been justified.</description><subject>Blackbody</subject><subject>Cosmology</subject><subject>Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Supernovae</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotj81Kw0AURgdBsNQ-gCsDLiV15t7cycxSgj-Fgot2H27NjLQ0mThJinl7Y-vq2xw-zhHiTsllZojkE8ef_WmpSMJS6tyaKzEDRJWaDOBGLLruIKUEnQMRzsTjph-qMQk-2Qyti004sUtWdRtiz02f-BCTInR1OIav8VZcez52bvG_c7F9fdkW7-n6421VPK9TJsC00jtGrjzhzjqZO5AZOVaZ8fxpQXnMLTBZqBwxGqhQIyNNzCSrtAWci_vL7bmkbOO-5jiWf0XluWgiHi5EG8P34Lq-PIQhNpNTCdIoZVHniL8U7ky5</recordid><startdate>20150224</startdate><enddate>20150224</enddate><creator>Baklanov, P V</creator><creator>Blinnikov, S I</creator><creator>M Sh Potashov</creator><creator>Dolgov, A D</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20150224</creationdate><title>Study of Supernovae Important for Cosmology</title><author>Baklanov, P V ; Blinnikov, S I ; M Sh Potashov ; Dolgov, A D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a523-d6ba3adf53b9e07e2045ea148fac921f3792a592de5a382d363a3545e67916923</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Blackbody</topic><topic>Cosmology</topic><topic>Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - High Energy Physics - Phenomenology</topic><topic>Supernovae</topic><toplevel>online_resources</toplevel><creatorcontrib>Baklanov, P V</creatorcontrib><creatorcontrib>Blinnikov, S I</creatorcontrib><creatorcontrib>M Sh Potashov</creatorcontrib><creatorcontrib>Dolgov, A D</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Baklanov, P V</au><au>Blinnikov, S I</au><au>M Sh Potashov</au><au>Dolgov, A D</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Study of Supernovae Important for Cosmology</atitle><jtitle>arXiv.org</jtitle><date>2015-02-24</date><risdate>2015</risdate><eissn>2331-8422</eissn><abstract>The dense shell method for the determination of distances to type IIn supernovae has been briefly reviewed. Applying our method to SN 2006gy, SN 2009ip, and SN 2010jl supernovae, we have obtained distances in excellent agreement with the previously known distances to the parent galaxies. The dense shell method is based on the radiation hydrodynamic model of a supernova. The method of the blackbody model, as well as the correctness of its application for simple estimates of distances from observation data, has been justified.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1502.06798</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2015-02 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_1502_06798 |
source | Freely Accessible Journals; arXiv.org |
subjects | Blackbody Cosmology Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Phenomenology Supernovae |
title | Study of Supernovae Important for Cosmology |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T22%3A47%3A15IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Study%20of%20Supernovae%20Important%20for%20Cosmology&rft.jtitle=arXiv.org&rft.au=Baklanov,%20P%20V&rft.date=2015-02-24&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1502.06798&rft_dat=%3Cproquest_arxiv%3E2081193673%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2081193673&rft_id=info:pmid/&rfr_iscdi=true |