Warm molecular gas in nearby galaxies. Mapping of the CO(3-2) emission

Using the Heinrich-Hertz-Telescope on Mt. Graham, Arizona, we have observed several nearby galaxies in the CO(3-2) line. The CO(3-2) emission traces - in contrast to lower rotational transitions - a warmer and denser component of the molecular gas. We find that this emission is spatially extended in...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2000-12
1. Verfasser: Dumke, Michael
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 Dumke, Michael
description Using the Heinrich-Hertz-Telescope on Mt. Graham, Arizona, we have observed several nearby galaxies in the CO(3-2) line. The CO(3-2) emission traces - in contrast to lower rotational transitions - a warmer and denser component of the molecular gas. We find that this emission is spatially extended in the target galaxies. The excitation conditions seem to vary with the location of the gas within the galaxy, and also with the overall properties of the target objects. However, a clear correlation between the CO(3-2) emission and other quantities, such as Hubble type or IR luminosity, is not present.
format Article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2092612643</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2092612643</sourcerecordid><originalsourceid>FETCH-proquest_journals_20926126433</originalsourceid><addsrcrecordid>eNqNisEKgkAUAJcgSMp_eNClDsb6Vq3OknSJLoFH2WK1lXXX9inU3-ehD-g0DDMzFqAQcXRIEBcsJGo555jtMU1FwIpS-g46Z9RjNNJDIwm0Baukv38mM_KtFe3gIvte2wZcDcNTQX7diAi3oDpNpJ1dsXktDanwxyVbF6dbfo56716joqFq3ejtlCrkR8xizBIh_ru--KI5eQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2092612643</pqid></control><display><type>article</type><title>Warm molecular gas in nearby galaxies. Mapping of the CO(3-2) emission</title><source>Free E- Journals</source><creator>Dumke, Michael</creator><creatorcontrib>Dumke, Michael</creatorcontrib><description>Using the Heinrich-Hertz-Telescope on Mt. Graham, Arizona, we have observed several nearby galaxies in the CO(3-2) line. The CO(3-2) emission traces - in contrast to lower rotational transitions - a warmer and denser component of the molecular gas. We find that this emission is spatially extended in the target galaxies. The excitation conditions seem to vary with the location of the gas within the galaxy, and also with the overall properties of the target objects. However, a clear correlation between the CO(3-2) emission and other quantities, such as Hubble type or IR luminosity, is not present.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Emission ; Galaxies ; Luminosity ; Mapping ; Molecular gases</subject><ispartof>arXiv.org, 2000-12</ispartof><rights>2000. This work is published under https://arxiv.org/licenses/assumed-1991-2003/license.html (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</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>776,780</link.rule.ids></links><search><creatorcontrib>Dumke, Michael</creatorcontrib><title>Warm molecular gas in nearby galaxies. Mapping of the CO(3-2) emission</title><title>arXiv.org</title><description>Using the Heinrich-Hertz-Telescope on Mt. Graham, Arizona, we have observed several nearby galaxies in the CO(3-2) line. The CO(3-2) emission traces - in contrast to lower rotational transitions - a warmer and denser component of the molecular gas. We find that this emission is spatially extended in the target galaxies. The excitation conditions seem to vary with the location of the gas within the galaxy, and also with the overall properties of the target objects. However, a clear correlation between the CO(3-2) emission and other quantities, such as Hubble type or IR luminosity, is not present.</description><subject>Emission</subject><subject>Galaxies</subject><subject>Luminosity</subject><subject>Mapping</subject><subject>Molecular gases</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqNisEKgkAUAJcgSMp_eNClDsb6Vq3OknSJLoFH2WK1lXXX9inU3-ehD-g0DDMzFqAQcXRIEBcsJGo555jtMU1FwIpS-g46Z9RjNNJDIwm0Baukv38mM_KtFe3gIvte2wZcDcNTQX7diAi3oDpNpJ1dsXktDanwxyVbF6dbfo56716joqFq3ejtlCrkR8xizBIh_ru--KI5eQ</recordid><startdate>20001207</startdate><enddate>20001207</enddate><creator>Dumke, Michael</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></search><sort><creationdate>20001207</creationdate><title>Warm molecular gas in nearby galaxies. Mapping of the CO(3-2) emission</title><author>Dumke, Michael</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20926126433</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>Emission</topic><topic>Galaxies</topic><topic>Luminosity</topic><topic>Mapping</topic><topic>Molecular gases</topic><toplevel>online_resources</toplevel><creatorcontrib>Dumke, Michael</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; 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></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Dumke, Michael</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Warm molecular gas in nearby galaxies. Mapping of the CO(3-2) emission</atitle><jtitle>arXiv.org</jtitle><date>2000-12-07</date><risdate>2000</risdate><eissn>2331-8422</eissn><abstract>Using the Heinrich-Hertz-Telescope on Mt. Graham, Arizona, we have observed several nearby galaxies in the CO(3-2) line. The CO(3-2) emission traces - in contrast to lower rotational transitions - a warmer and denser component of the molecular gas. We find that this emission is spatially extended in the target galaxies. The excitation conditions seem to vary with the location of the gas within the galaxy, and also with the overall properties of the target objects. However, a clear correlation between the CO(3-2) emission and other quantities, such as Hubble type or IR luminosity, is not present.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2000-12
issn 2331-8422
language eng
recordid cdi_proquest_journals_2092612643
source Free E- Journals
subjects Emission
Galaxies
Luminosity
Mapping
Molecular gases
title Warm molecular gas in nearby galaxies. Mapping of the CO(3-2) emission
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-30T10%3A00%3A00IST&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:book&rft.genre=document&rft.atitle=Warm%20molecular%20gas%20in%20nearby%20galaxies.%20Mapping%20of%20the%20CO(3-2)%20emission&rft.jtitle=arXiv.org&rft.au=Dumke,%20Michael&rft.date=2000-12-07&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2092612643%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2092612643&rft_id=info:pmid/&rfr_iscdi=true