Methods to Account for Interstellar Extinction

Methods to Account for Interstellar Extinction

A detailed knowledge of the galactic extinction is mandatory to obtain the time variation of the astrophysical/kinematical parameters outside the solar neighborhood. One may hope that the GAIA photometry itself will contribute color excesses for most of the studied objects, otherwise the extinction...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astrophysics and space science 2002-01, Vol.280 (1-2), p.97-107
1. Verfasser: Knude, Jens
Format: Artikel
Sprache:eng
Schlagworte:
Astrophysics
Methods
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 107
container_issue 1-2
container_start_page 97
container_title Astrophysics and space science
container_volume 280
creator Knude, Jens
description A detailed knowledge of the galactic extinction is mandatory to obtain the time variation of the astrophysical/kinematical parameters outside the solar neighborhood. One may hope that the GAIA photometry itself will contribute color excesses for most of the studied objects, otherwise the extinction must be deduced from the external sources. 3-Dgalactic models where the dust distribution is an integral part seems to be a viable solution. Some statistical information may be obtained even from a color vs. distance diagrams.[PUBLICATION ABSTRACT]
doi_str_mv 10.1023/A:1015522710665
format Article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_miscellaneous_807263693</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>807263693</sourcerecordid><originalsourceid>FETCH-LOGICAL-p274t-bbde18c7d7813f5155b4bd619ee6d2a73a49095d793aaf5f21732bd318599aff3</originalsourceid><addsrcrecordid>eNqF0E1LxDAQBuAgCtbVs9fiQU9dM_mOt2VZdWHFi8LeStok2KU2a5OCP98sevKgp2HgYeadQegS8BwwobeLO8DAOSESsBD8CBXAJak0E9tjVGCMWSUY3p6isxh3udVCywLNn1x6CzaWKZSLtg3TkEofxnI9JDfG5PrejOXqM3VDm7ownKMTb_roLn7qDL3er16Wj9Xm-WG9XGyqPZEsVU1jHahWWqmAep5jNayxArRzwhIjqWEaa26lpsZ47glIShpLQXGtjfd0hm6-5-7H8DG5mOr3LraHNIMLU6wVlkRQoWmW139KInl-Axb_wrxbgYIDvPoFd2Eah3xuLTlWTIBg9AsYwmzl</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>750846164</pqid></control><display><type>article</type><title>Methods to Account for Interstellar Extinction</title><source>SpringerLink Journals</source><creator>Knude, Jens</creator><creatorcontrib>Knude, Jens</creatorcontrib><description>A detailed knowledge of the galactic extinction is mandatory to obtain the time variation of the astrophysical/kinematical parameters outside the solar neighborhood. One may hope that the GAIA photometry itself will contribute color excesses for most of the studied objects, otherwise the extinction must be deduced from the external sources. 3-Dgalactic models where the dust distribution is an integral part seems to be a viable solution. Some statistical information may be obtained even from a color vs. distance diagrams.[PUBLICATION ABSTRACT]</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1023/A:1015522710665</identifier><language>eng</language><publisher>Dordrecht: Springer Nature B.V</publisher><subject>Astrophysics ; Methods</subject><ispartof>Astrophysics and space science, 2002-01, Vol.280 (1-2), p.97-107</ispartof><rights>Kluwer Academic Publishers 2002</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Knude, Jens</creatorcontrib><title>Methods to Account for Interstellar Extinction</title><title>Astrophysics and space science</title><description>A detailed knowledge of the galactic extinction is mandatory to obtain the time variation of the astrophysical/kinematical parameters outside the solar neighborhood. One may hope that the GAIA photometry itself will contribute color excesses for most of the studied objects, otherwise the extinction must be deduced from the external sources. 3-Dgalactic models where the dust distribution is an integral part seems to be a viable solution. Some statistical information may be obtained even from a color vs. distance diagrams.[PUBLICATION ABSTRACT]</description><subject>Astrophysics</subject><subject>Methods</subject><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqF0E1LxDAQBuAgCtbVs9fiQU9dM_mOt2VZdWHFi8LeStok2KU2a5OCP98sevKgp2HgYeadQegS8BwwobeLO8DAOSESsBD8CBXAJak0E9tjVGCMWSUY3p6isxh3udVCywLNn1x6CzaWKZSLtg3TkEofxnI9JDfG5PrejOXqM3VDm7ownKMTb_roLn7qDL3er16Wj9Xm-WG9XGyqPZEsVU1jHahWWqmAep5jNayxArRzwhIjqWEaa26lpsZ47glIShpLQXGtjfd0hm6-5-7H8DG5mOr3LraHNIMLU6wVlkRQoWmW139KInl-Axb_wrxbgYIDvPoFd2Eah3xuLTlWTIBg9AsYwmzl</recordid><startdate>20020101</startdate><enddate>20020101</enddate><creator>Knude, Jens</creator><general>Springer Nature B.V</general><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20020101</creationdate><title>Methods to Account for Interstellar Extinction</title><author>Knude, Jens</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p274t-bbde18c7d7813f5155b4bd619ee6d2a73a49095d793aaf5f21732bd318599aff3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2002</creationdate><topic>Astrophysics</topic><topic>Methods</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Knude, Jens</creatorcontrib><collection>ProQuest Central (Corporate)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies &amp; Aerospace Collection</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>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies &amp; Aerospace Database</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</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 Basic</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Knude, Jens</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Methods to Account for Interstellar Extinction</atitle><jtitle>Astrophysics and space science</jtitle><date>2002-01-01</date><risdate>2002</risdate><volume>280</volume><issue>1-2</issue><spage>97</spage><epage>107</epage><pages>97-107</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>A detailed knowledge of the galactic extinction is mandatory to obtain the time variation of the astrophysical/kinematical parameters outside the solar neighborhood. One may hope that the GAIA photometry itself will contribute color excesses for most of the studied objects, otherwise the extinction must be deduced from the external sources. 3-Dgalactic models where the dust distribution is an integral part seems to be a viable solution. Some statistical information may be obtained even from a color vs. distance diagrams.[PUBLICATION ABSTRACT]</abstract><cop>Dordrecht</cop><pub>Springer Nature B.V</pub><doi>10.1023/A:1015522710665</doi><tpages>11</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0004-640X
ispartof Astrophysics and space science, 2002-01, Vol.280 (1-2), p.97-107
issn 0004-640X
1572-946X
language eng
recordid cdi_proquest_miscellaneous_807263693
source SpringerLink Journals
subjects Astrophysics
Methods
title Methods to Account for Interstellar Extinction
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-04T23%3A42%3A36IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Methods%20to%20Account%20for%20Interstellar%20Extinction&rft.jtitle=Astrophysics%20and%20space%20science&rft.au=Knude,%20Jens&rft.date=2002-01-01&rft.volume=280&rft.issue=1-2&rft.spage=97&rft.epage=107&rft.pages=97-107&rft.issn=0004-640X&rft.eissn=1572-946X&rft_id=info:doi/10.1023/A:1015522710665&rft_dat=%3Cproquest%3E807263693%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=750846164&rft_id=info:pmid/&rfr_iscdi=true