Molecular cloud distance determination from deep NIR survey extinction measurements
Using near-infrared United Kingdom Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey data, we make extinction measurements to individual stars along the same line of sight as molecular clouds. Using an existing 3D extinction map of the inner Galaxy, that provides line of sight specific extinct...
Gespeichert in:
| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2010-09, Vol.407 (2), p.923-936 |
|---|---|
| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 936 |
|---|---|
| container_issue | 2 |
| container_start_page | 923 |
| container_title | Monthly notices of the Royal Astronomical Society |
| container_volume | 407 |
| creator | Stead, J. J. Hoare, M. G. |
| description | Using near-infrared United Kingdom Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey data, we make extinction measurements to individual stars along the same line of sight as molecular clouds. Using an existing 3D extinction map of the inner Galaxy, that provides line of sight specific extinction–distance relationships, we convert the measured extinction of molecular clouds to a corresponding distance. These distances are derived independently from kinematic methods, typically used to derive distances to molecular clouds, and as such they have no near/far ambiguity. The near/far distance ambiguity has been resolved for 27 clouds, and distances have been derived to 20 clouds. The results are found to be in good agreement with kinematic measurements to molecular clouds where the ambiguity has already been resolved, using H i self-absorption techniques. |
| doi_str_mv | 10.1111/j.1365-2966.2010.17014.x |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_wiley</sourceid><recordid>TN_cdi_proquest_miscellaneous_807285508</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><oup_id>10.1111/j.1365-2966.2010.17014.x</oup_id><sourcerecordid>2127083271</sourcerecordid><originalsourceid>FETCH-LOGICAL-c4564-eabded8e5b2bd592e66124876857482e1b740970db9dd62f4268899e23cefeb13</originalsourceid><addsrcrecordid>eNp1kEtrGzEUhUVpIG7S_zB009W4kkav2RSKae1AXiQpCd5cNKNrGHcerjST2v8-Grt4kZC70eXccw7iIyRhdMrifFtPWaZkynOlppyOqqZMTLcfyOR4-EgmlGYyNZqxU_IphDWlVGRcTcj9VVdjOdTWJ2XdDS5xVehtW2LisEffVK3tq65NVr5rooSb5PriLgmDf8Zdgtu-asv9vUEbRWyw7cM5OVnZOuDn_-8Z-f3r58NskV7ezC9mPy7TUkglUrSFQ2dQFrxwMueoFOPCaGWkFoYjK7SguaauyJ1TfCW4MibPkWclrrBg2Rn5eujd-O7vgKGHpgol1rVtsRsCGKq5kZKa6PzyyrnuBt_Gz4EWOadGSBpN3w-mf1WNO9j4qrF-B4zCCBrWMPKEkSeMoGEPGrZwdX23X2NBdijohs078fRNPKbSQyqCx-0xZ_0fUDrTEhZPS5g_zW71_fIWHrMX2UmSyQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>749208450</pqid></control><display><type>article</type><title>Molecular cloud distance determination from deep NIR survey extinction measurements</title><source>Wiley Online Library Journals Frontfile Complete</source><source>Oxford Academic Journals (Open Access)</source><creator>Stead, J. J. ; Hoare, M. G.</creator><creatorcontrib>Stead, J. J. ; Hoare, M. G.</creatorcontrib><description>Using near-infrared United Kingdom Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey data, we make extinction measurements to individual stars along the same line of sight as molecular clouds. Using an existing 3D extinction map of the inner Galaxy, that provides line of sight specific extinction–distance relationships, we convert the measured extinction of molecular clouds to a corresponding distance. These distances are derived independently from kinematic methods, typically used to derive distances to molecular clouds, and as such they have no near/far ambiguity. The near/far distance ambiguity has been resolved for 27 clouds, and distances have been derived to 20 clouds. The results are found to be in good agreement with kinematic measurements to molecular clouds where the ambiguity has already been resolved, using H i self-absorption techniques.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1111/j.1365-2966.2010.17014.x</identifier><language>eng</language><publisher>Oxford, UK: Blackwell Publishing Ltd</publisher><subject>Dust ; dust, extinction ; extinction ; Infrared imaging systems ; ISM: general ; Star maps ; Stars & galaxies</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2010-09, Vol.407 (2), p.923-936</ispartof><rights>2010 The Authors. Journal compilation © 2010 RAS 2010</rights><rights>2010 The Authors. Journal compilation © 2010 RAS</rights><rights>Journal compilation © 2010 RAS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4564-eabded8e5b2bd592e66124876857482e1b740970db9dd62f4268899e23cefeb13</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1111%2Fj.1365-2966.2010.17014.x$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1111%2Fj.1365-2966.2010.17014.x$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,27901,27902,45550,45551</link.rule.ids></links><search><creatorcontrib>Stead, J. J.</creatorcontrib><creatorcontrib>Hoare, M. G.</creatorcontrib><title>Molecular cloud distance determination from deep NIR survey extinction measurements</title><title>Monthly notices of the Royal Astronomical Society</title><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><description>Using near-infrared United Kingdom Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey data, we make extinction measurements to individual stars along the same line of sight as molecular clouds. Using an existing 3D extinction map of the inner Galaxy, that provides line of sight specific extinction–distance relationships, we convert the measured extinction of molecular clouds to a corresponding distance. These distances are derived independently from kinematic methods, typically used to derive distances to molecular clouds, and as such they have no near/far ambiguity. The near/far distance ambiguity has been resolved for 27 clouds, and distances have been derived to 20 clouds. The results are found to be in good agreement with kinematic measurements to molecular clouds where the ambiguity has already been resolved, using H i self-absorption techniques.</description><subject>Dust</subject><subject>dust, extinction</subject><subject>extinction</subject><subject>Infrared imaging systems</subject><subject>ISM: general</subject><subject>Star maps</subject><subject>Stars & galaxies</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp1kEtrGzEUhUVpIG7S_zB009W4kkav2RSKae1AXiQpCd5cNKNrGHcerjST2v8-Grt4kZC70eXccw7iIyRhdMrifFtPWaZkynOlppyOqqZMTLcfyOR4-EgmlGYyNZqxU_IphDWlVGRcTcj9VVdjOdTWJ2XdDS5xVehtW2LisEffVK3tq65NVr5rooSb5PriLgmDf8Zdgtu-asv9vUEbRWyw7cM5OVnZOuDn_-8Z-f3r58NskV7ezC9mPy7TUkglUrSFQ2dQFrxwMueoFOPCaGWkFoYjK7SguaauyJ1TfCW4MibPkWclrrBg2Rn5eujd-O7vgKGHpgol1rVtsRsCGKq5kZKa6PzyyrnuBt_Gz4EWOadGSBpN3w-mf1WNO9j4qrF-B4zCCBrWMPKEkSeMoGEPGrZwdX23X2NBdijohs078fRNPKbSQyqCx-0xZ_0fUDrTEhZPS5g_zW71_fIWHrMX2UmSyQ</recordid><startdate>201009</startdate><enddate>201009</enddate><creator>Stead, J. J.</creator><creator>Hoare, M. G.</creator><general>Blackwell Publishing Ltd</general><general>Oxford University Press</general><scope>BSCLL</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>201009</creationdate><title>Molecular cloud distance determination from deep NIR survey extinction measurements</title><author>Stead, J. J. ; Hoare, M. G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4564-eabded8e5b2bd592e66124876857482e1b740970db9dd62f4268899e23cefeb13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Dust</topic><topic>dust, extinction</topic><topic>extinction</topic><topic>Infrared imaging systems</topic><topic>ISM: general</topic><topic>Star maps</topic><topic>Stars & galaxies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Stead, J. J.</creatorcontrib><creatorcontrib>Hoare, M. G.</creatorcontrib><collection>Istex</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Stead, J. J.</au><au>Hoare, M. G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Molecular cloud distance determination from deep NIR survey extinction measurements</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><stitle>Monthly Notices of the Royal Astronomical Society</stitle><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><date>2010-09</date><risdate>2010</risdate><volume>407</volume><issue>2</issue><spage>923</spage><epage>936</epage><pages>923-936</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>Using near-infrared United Kingdom Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey data, we make extinction measurements to individual stars along the same line of sight as molecular clouds. Using an existing 3D extinction map of the inner Galaxy, that provides line of sight specific extinction–distance relationships, we convert the measured extinction of molecular clouds to a corresponding distance. These distances are derived independently from kinematic methods, typically used to derive distances to molecular clouds, and as such they have no near/far ambiguity. The near/far distance ambiguity has been resolved for 27 clouds, and distances have been derived to 20 clouds. The results are found to be in good agreement with kinematic measurements to molecular clouds where the ambiguity has already been resolved, using H i self-absorption techniques.</abstract><cop>Oxford, UK</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1111/j.1365-2966.2010.17014.x</doi><tpages>14</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0035-8711 |
| ispartof | Monthly notices of the Royal Astronomical Society, 2010-09, Vol.407 (2), p.923-936 |
| issn | 0035-8711 1365-2966 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_807285508 |
| source | Wiley Online Library Journals Frontfile Complete; Oxford Academic Journals (Open Access) |
| subjects | Dust dust, extinction extinction Infrared imaging systems ISM: general Star maps Stars & galaxies |
| title | Molecular cloud distance determination from deep NIR survey extinction measurements |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-04T18%3A37%3A38IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_wiley&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Molecular%20cloud%20distance%20determination%20from%20deep%20NIR%20survey%20extinction%20measurements&rft.jtitle=Monthly%20notices%20of%20the%20Royal%20Astronomical%20Society&rft.au=Stead,%20J.%20J.&rft.date=2010-09&rft.volume=407&rft.issue=2&rft.spage=923&rft.epage=936&rft.pages=923-936&rft.issn=0035-8711&rft.eissn=1365-2966&rft_id=info:doi/10.1111/j.1365-2966.2010.17014.x&rft_dat=%3Cproquest_wiley%3E2127083271%3C/proquest_wiley%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=749208450&rft_id=info:pmid/&rft_oup_id=10.1111/j.1365-2966.2010.17014.x&rfr_iscdi=true |