Loading…
Chandra HETG Spectra of SN 1987A at 20 Years
We have undertaken deep, high-resolution observations of SN 1987A at approximately 20 years after its explosion with the Chandra HETG and LETG spectrometers. Here we present the HETG X-ray spectra of SN 1987A having unprecedented spectral resolution and signal-to-noise ratios in the 6-20 AA bandpass...
Saved in:
Published in: | The Astrophysical journal 2008-04, Vol.676 (2), p.L131-L134 |
---|---|
Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653 |
---|---|
cites | cdi_FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653 |
container_end_page | L134 |
container_issue | 2 |
container_start_page | L131 |
container_title | The Astrophysical journal |
container_volume | 676 |
creator | Dewey, D Zhekov, S. A McCray, R Canizares, C. R |
description | We have undertaken deep, high-resolution observations of SN 1987A at approximately 20 years after its explosion with the Chandra HETG and LETG spectrometers. Here we present the HETG X-ray spectra of SN 1987A having unprecedented spectral resolution and signal-to-noise ratios in the 6-20 AA bandpass, which includes the H-like and He-like lines of Si, Mg, and Ne, as well as 0 vIII lines and bright Fe xvII lines. In joint analysis with LETG data, we find that there has been a significant decrease from 2004 to 2007 in the average temperature of the highest temperature component of the shocked-plasma emission. Model fitting of the profiles of individual HETG lines yields bulk kinematic velocities of the higher-Z ions, Mg and Si, that are significantly lower than those inferred from the LETG 2004 observations. |
doi_str_mv | 10.1086/587549 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_20865897</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>20865897</sourcerecordid><originalsourceid>FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653</originalsourceid><addsrcrecordid>eNp90E1LAzEQBuAgCtaqv2E9qAddnSSbr2MptRWKHloPnkKaTXBl212T7cF_b0qLVRBPMwMP78CL0DmGOwyS3zMpWKEOUA8zKvOCMnH4Yz9GJzG-A0BBlOqh2-GbWZXBZJPRfJzNWme7dDQ-mz1lWEkxyEyXEchenQnxFB15U0d3tpt99PIwmg8n-fR5_DgcTHNbYOjyhWSKSOu9AoItYEeY8pwwrjD3wptSGgmEUSpLUzBLFQeXAOMLLxbAGe2j621uG5qPtYudXlbRuro2K9esoxYFxVgqJpO8-leSVAiTSuyhDU2MwXndhmppwqfGoDe16W1tCV7uEk20pvbBrGwVvzUBQgQWm883W1c17T4rtaw3LWsuuCZ6iinWbemTvvhD__78BU14fbo</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>20865897</pqid></control><display><type>article</type><title>Chandra HETG Spectra of SN 1987A at 20 Years</title><source>EZB Electronic Journals Library</source><creator>Dewey, D ; Zhekov, S. A ; McCray, R ; Canizares, C. R</creator><creatorcontrib>Dewey, D ; Zhekov, S. A ; McCray, R ; Canizares, C. R</creatorcontrib><description>We have undertaken deep, high-resolution observations of SN 1987A at approximately 20 years after its explosion with the Chandra HETG and LETG spectrometers. Here we present the HETG X-ray spectra of SN 1987A having unprecedented spectral resolution and signal-to-noise ratios in the 6-20 AA bandpass, which includes the H-like and He-like lines of Si, Mg, and Ne, as well as 0 vIII lines and bright Fe xvII lines. In joint analysis with LETG data, we find that there has been a significant decrease from 2004 to 2007 in the average temperature of the highest temperature component of the shocked-plasma emission. Model fitting of the profiles of individual HETG lines yields bulk kinematic velocities of the higher-Z ions, Mg and Si, that are significantly lower than those inferred from the LETG 2004 observations.</description><identifier>ISSN: 1538-4357</identifier><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/587549</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Chicago, IL: IOP Publishing</publisher><subject>Astronomy ; Earth, ocean, space ; Exact sciences and technology</subject><ispartof>The Astrophysical journal, 2008-04, Vol.676 (2), p.L131-L134</ispartof><rights>2008 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653</citedby><cites>FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=20227178$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Dewey, D</creatorcontrib><creatorcontrib>Zhekov, S. A</creatorcontrib><creatorcontrib>McCray, R</creatorcontrib><creatorcontrib>Canizares, C. R</creatorcontrib><title>Chandra HETG Spectra of SN 1987A at 20 Years</title><title>The Astrophysical journal</title><description>We have undertaken deep, high-resolution observations of SN 1987A at approximately 20 years after its explosion with the Chandra HETG and LETG spectrometers. Here we present the HETG X-ray spectra of SN 1987A having unprecedented spectral resolution and signal-to-noise ratios in the 6-20 AA bandpass, which includes the H-like and He-like lines of Si, Mg, and Ne, as well as 0 vIII lines and bright Fe xvII lines. In joint analysis with LETG data, we find that there has been a significant decrease from 2004 to 2007 in the average temperature of the highest temperature component of the shocked-plasma emission. Model fitting of the profiles of individual HETG lines yields bulk kinematic velocities of the higher-Z ions, Mg and Si, that are significantly lower than those inferred from the LETG 2004 observations.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><issn>1538-4357</issn><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNp90E1LAzEQBuAgCtaqv2E9qAddnSSbr2MptRWKHloPnkKaTXBl212T7cF_b0qLVRBPMwMP78CL0DmGOwyS3zMpWKEOUA8zKvOCMnH4Yz9GJzG-A0BBlOqh2-GbWZXBZJPRfJzNWme7dDQ-mz1lWEkxyEyXEchenQnxFB15U0d3tpt99PIwmg8n-fR5_DgcTHNbYOjyhWSKSOu9AoItYEeY8pwwrjD3wptSGgmEUSpLUzBLFQeXAOMLLxbAGe2j621uG5qPtYudXlbRuro2K9esoxYFxVgqJpO8-leSVAiTSuyhDU2MwXndhmppwqfGoDe16W1tCV7uEk20pvbBrGwVvzUBQgQWm883W1c17T4rtaw3LWsuuCZ6iinWbemTvvhD__78BU14fbo</recordid><startdate>20080401</startdate><enddate>20080401</enddate><creator>Dewey, D</creator><creator>Zhekov, S. A</creator><creator>McCray, R</creator><creator>Canizares, C. R</creator><general>IOP Publishing</general><general>University of Chicago Press</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20080401</creationdate><title>Chandra HETG Spectra of SN 1987A at 20 Years</title><author>Dewey, D ; Zhekov, S. A ; McCray, R ; Canizares, C. R</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><topic>Astronomy</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Dewey, D</creatorcontrib><creatorcontrib>Zhekov, S. A</creatorcontrib><creatorcontrib>McCray, R</creatorcontrib><creatorcontrib>Canizares, C. R</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dewey, D</au><au>Zhekov, S. A</au><au>McCray, R</au><au>Canizares, C. R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Chandra HETG Spectra of SN 1987A at 20 Years</atitle><jtitle>The Astrophysical journal</jtitle><date>2008-04-01</date><risdate>2008</risdate><volume>676</volume><issue>2</issue><spage>L131</spage><epage>L134</epage><pages>L131-L134</pages><issn>1538-4357</issn><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>We have undertaken deep, high-resolution observations of SN 1987A at approximately 20 years after its explosion with the Chandra HETG and LETG spectrometers. Here we present the HETG X-ray spectra of SN 1987A having unprecedented spectral resolution and signal-to-noise ratios in the 6-20 AA bandpass, which includes the H-like and He-like lines of Si, Mg, and Ne, as well as 0 vIII lines and bright Fe xvII lines. In joint analysis with LETG data, we find that there has been a significant decrease from 2004 to 2007 in the average temperature of the highest temperature component of the shocked-plasma emission. Model fitting of the profiles of individual HETG lines yields bulk kinematic velocities of the higher-Z ions, Mg and Si, that are significantly lower than those inferred from the LETG 2004 observations.</abstract><cop>Chicago, IL</cop><pub>IOP Publishing</pub><doi>10.1086/587549</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1538-4357 |
ispartof | The Astrophysical journal, 2008-04, Vol.676 (2), p.L131-L134 |
issn | 1538-4357 0004-637X 1538-4357 |
language | eng |
recordid | cdi_proquest_miscellaneous_20865897 |
source | EZB Electronic Journals Library |
subjects | Astronomy Earth, ocean, space Exact sciences and technology |
title | Chandra HETG Spectra of SN 1987A at 20 Years |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T14%3A32%3A36IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Chandra%20HETG%20Spectra%20of%20SN%201987A%20at%2020%20Years&rft.jtitle=The%20Astrophysical%20journal&rft.au=Dewey,%20D&rft.date=2008-04-01&rft.volume=676&rft.issue=2&rft.spage=L131&rft.epage=L134&rft.pages=L131-L134&rft.issn=1538-4357&rft.eissn=1538-4357&rft.coden=ASJOAB&rft_id=info:doi/10.1086/587549&rft_dat=%3Cproquest_cross%3E20865897%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c410t-b85928cff9021c01e259f6256916f7fad8a8025338da45c3960e9f656bf7b0653%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=20865897&rft_id=info:pmid/&rfr_iscdi=true |