A Galactic Plane Survey in the CO (2-1) Line with the 60 cm Telescopes to Address Physical Condition of the Interstellar Matter
To address its temperature and density we made observations of the galactic plane in CO (2-1) line with VST1 and VST2. Using a kinetic model we estimate the volume emissivities and the line intensity ratio as a function of galactocentric radius. Using data in the first and 4th quadrants separately w...
Gespeichert in:
| Veröffentlicht in: | Symposium - International Astronomical Union 2002, Vol.199, p.339-340 |
|---|---|
| Hauptverfasser: | , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 340 |
|---|---|
| container_issue | |
| container_start_page | 339 |
| container_title | Symposium - International Astronomical Union |
| container_volume | 199 |
| creator | Handa, T. Hasegawa, T. Morino, J.I. Sawada, T. Sakamoto, S. Usuda, K.S. Luna, A. Bronfman, L. Hayashi, M. |
| description | To address its temperature and density we made observations of the galactic plane in CO (2-1) line with VST1 and VST2. Using a kinetic model we estimate the volume emissivities and the line intensity ratio as a function of galactocentric radius. Using data in the first and 4th quadrants separately we got shallow gradient in the both quadrants; at the smaller radius is the higher in ratio. The gradient is contributed by less bright pixels in the l-v diagram, suggesting molecular gas in interarm is different along the galactocentric radius but in arm is not. |
| doi_str_mv | 10.1017/S0074180900169256 |
| format | Article |
| fullrecord | <record><control><sourceid>crossref</sourceid><recordid>TN_cdi_crossref_primary_10_1017_S0074180900169256</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1017_S0074180900169256</sourcerecordid><originalsourceid>FETCH-LOGICAL-c856-54adcfc7ee6945916c779d21fe45658c5eb9a68c2b0cecaa535b444b19d8e543</originalsourceid><addsrcrecordid>eNplkDFPwzAUhD2ARFX6A9jeCEPATm3HHqsISqWiVmr3yHl5UY3SpLINqBN_nbawMZ3uO90Nx9id4I-Ci-Jpw3khheGWc6FtrvQVG51RdmY3bBLjOz9FylhjxIh9z2DuOofJI6w71xNsPsInHcH3kHYE5Qru80w8wNKfsi-fdhesOeAettRRxOFAEdIAs6YJFCOsd8fo0XVQDn3jkx96GNpLa9EnCjFR17kAby6d3C27bl0XafKnY7Z5ed6Wr9lyNV-Us2WGRulMSddgiwWRtlJZobEobJOLlqTSyqCi2jptMK85EjqnpqqWUtbCNoaUnI6Z-F3FMMQYqK0Owe9dOFaCV-fbqn-3TX8A1WBg_g</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>A Galactic Plane Survey in the CO (2-1) Line with the 60 cm Telescopes to Address Physical Condition of the Interstellar Matter</title><source>Alma/SFX Local Collection</source><creator>Handa, T. ; Hasegawa, T. ; Morino, J.I. ; Sawada, T. ; Sakamoto, S. ; Usuda, K.S. ; Luna, A. ; Bronfman, L. ; Hayashi, M.</creator><creatorcontrib>Handa, T. ; Hasegawa, T. ; Morino, J.I. ; Sawada, T. ; Sakamoto, S. ; Usuda, K.S. ; Luna, A. ; Bronfman, L. ; Hayashi, M.</creatorcontrib><description>To address its temperature and density we made observations of the galactic plane in CO (2-1) line with VST1 and VST2. Using a kinetic model we estimate the volume emissivities and the line intensity ratio as a function of galactocentric radius. Using data in the first and 4th quadrants separately we got shallow gradient in the both quadrants; at the smaller radius is the higher in ratio. The gradient is contributed by less bright pixels in the l-v diagram, suggesting molecular gas in interarm is different along the galactocentric radius but in arm is not.</description><identifier>ISSN: 0074-1809</identifier><identifier>DOI: 10.1017/S0074180900169256</identifier><language>eng</language><ispartof>Symposium - International Astronomical Union, 2002, Vol.199, p.339-340</ispartof><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c856-54adcfc7ee6945916c779d21fe45658c5eb9a68c2b0cecaa535b444b19d8e543</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,4010,27900,27901,27902</link.rule.ids></links><search><creatorcontrib>Handa, T.</creatorcontrib><creatorcontrib>Hasegawa, T.</creatorcontrib><creatorcontrib>Morino, J.I.</creatorcontrib><creatorcontrib>Sawada, T.</creatorcontrib><creatorcontrib>Sakamoto, S.</creatorcontrib><creatorcontrib>Usuda, K.S.</creatorcontrib><creatorcontrib>Luna, A.</creatorcontrib><creatorcontrib>Bronfman, L.</creatorcontrib><creatorcontrib>Hayashi, M.</creatorcontrib><title>A Galactic Plane Survey in the CO (2-1) Line with the 60 cm Telescopes to Address Physical Condition of the Interstellar Matter</title><title>Symposium - International Astronomical Union</title><description>To address its temperature and density we made observations of the galactic plane in CO (2-1) line with VST1 and VST2. Using a kinetic model we estimate the volume emissivities and the line intensity ratio as a function of galactocentric radius. Using data in the first and 4th quadrants separately we got shallow gradient in the both quadrants; at the smaller radius is the higher in ratio. The gradient is contributed by less bright pixels in the l-v diagram, suggesting molecular gas in interarm is different along the galactocentric radius but in arm is not.</description><issn>0074-1809</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><recordid>eNplkDFPwzAUhD2ARFX6A9jeCEPATm3HHqsISqWiVmr3yHl5UY3SpLINqBN_nbawMZ3uO90Nx9id4I-Ci-Jpw3khheGWc6FtrvQVG51RdmY3bBLjOz9FylhjxIh9z2DuOofJI6w71xNsPsInHcH3kHYE5Qru80w8wNKfsi-fdhesOeAettRRxOFAEdIAs6YJFCOsd8fo0XVQDn3jkx96GNpLa9EnCjFR17kAby6d3C27bl0XafKnY7Z5ed6Wr9lyNV-Us2WGRulMSddgiwWRtlJZobEobJOLlqTSyqCi2jptMK85EjqnpqqWUtbCNoaUnI6Z-F3FMMQYqK0Owe9dOFaCV-fbqn-3TX8A1WBg_g</recordid><startdate>2002</startdate><enddate>2002</enddate><creator>Handa, T.</creator><creator>Hasegawa, T.</creator><creator>Morino, J.I.</creator><creator>Sawada, T.</creator><creator>Sakamoto, S.</creator><creator>Usuda, K.S.</creator><creator>Luna, A.</creator><creator>Bronfman, L.</creator><creator>Hayashi, M.</creator><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>2002</creationdate><title>A Galactic Plane Survey in the CO (2-1) Line with the 60 cm Telescopes to Address Physical Condition of the Interstellar Matter</title><author>Handa, T. ; Hasegawa, T. ; Morino, J.I. ; Sawada, T. ; Sakamoto, S. ; Usuda, K.S. ; Luna, A. ; Bronfman, L. ; Hayashi, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c856-54adcfc7ee6945916c779d21fe45658c5eb9a68c2b0cecaa535b444b19d8e543</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2002</creationdate><toplevel>online_resources</toplevel><creatorcontrib>Handa, T.</creatorcontrib><creatorcontrib>Hasegawa, T.</creatorcontrib><creatorcontrib>Morino, J.I.</creatorcontrib><creatorcontrib>Sawada, T.</creatorcontrib><creatorcontrib>Sakamoto, S.</creatorcontrib><creatorcontrib>Usuda, K.S.</creatorcontrib><creatorcontrib>Luna, A.</creatorcontrib><creatorcontrib>Bronfman, L.</creatorcontrib><creatorcontrib>Hayashi, M.</creatorcontrib><collection>CrossRef</collection><jtitle>Symposium - International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Handa, T.</au><au>Hasegawa, T.</au><au>Morino, J.I.</au><au>Sawada, T.</au><au>Sakamoto, S.</au><au>Usuda, K.S.</au><au>Luna, A.</au><au>Bronfman, L.</au><au>Hayashi, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Galactic Plane Survey in the CO (2-1) Line with the 60 cm Telescopes to Address Physical Condition of the Interstellar Matter</atitle><jtitle>Symposium - International Astronomical Union</jtitle><date>2002</date><risdate>2002</risdate><volume>199</volume><spage>339</spage><epage>340</epage><pages>339-340</pages><issn>0074-1809</issn><abstract>To address its temperature and density we made observations of the galactic plane in CO (2-1) line with VST1 and VST2. Using a kinetic model we estimate the volume emissivities and the line intensity ratio as a function of galactocentric radius. Using data in the first and 4th quadrants separately we got shallow gradient in the both quadrants; at the smaller radius is the higher in ratio. The gradient is contributed by less bright pixels in the l-v diagram, suggesting molecular gas in interarm is different along the galactocentric radius but in arm is not.</abstract><doi>10.1017/S0074180900169256</doi><tpages>2</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0074-1809 |
| ispartof | Symposium - International Astronomical Union, 2002, Vol.199, p.339-340 |
| issn | 0074-1809 |
| language | eng |
| recordid | cdi_crossref_primary_10_1017_S0074180900169256 |
| source | Alma/SFX Local Collection |
| title | A Galactic Plane Survey in the CO (2-1) Line with the 60 cm Telescopes to Address Physical Condition of the Interstellar Matter |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-10T11%3A58%3A47IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20Galactic%20Plane%20Survey%20in%20the%20CO%20(2-1)%20Line%20with%20the%2060%20cm%20Telescopes%20to%20Address%20Physical%20Condition%20of%20the%20Interstellar%20Matter&rft.jtitle=Symposium%20-%20International%20Astronomical%20Union&rft.au=Handa,%20T.&rft.date=2002&rft.volume=199&rft.spage=339&rft.epage=340&rft.pages=339-340&rft.issn=0074-1809&rft_id=info:doi/10.1017/S0074180900169256&rft_dat=%3Ccrossref%3E10_1017_S0074180900169256%3C/crossref%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |