PMO OpenIR  > 分子云与恒星形成研究团组
Dense gas in nearby galaxies XIII. CO submillimeter line emission from the starburst galaxy M 82
Mao, RQ; Henkel, C; Schulz, A; Zielinsky, M; Mauersberger, R; Storzer, H; Wilson, TL; Gensheimer, P
2000-06-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume358Issue:2Pages:433-450
Abstract(CO)-C-12 J = 1-0, 2-1, 4-3, 7-6, and (CO)-C-13 1-0, 2-1, and 3-2 line emission was mapped with angular resolutions of 13 " - 22 " toward the nuclear region of the archetypical starburst galaxy M 82. There are two hotspots on either side of the dynamical center, with the south-western lobe being slightly more prominent. Lobe spacings are not identical for all transitions: For the submillimeter CO lines, the spacing is similar to 15 ", for the millimeter lines (CO J = 2-1 and 1-0) the spacing is similar to 26 ", indicating the presence of a 'low' and a 'high' CO excitation component.
KeywordGalaxies : Active Galaxies : Individual : M82 Galaxies : Ism Galaxies : Nuclei Galaxies : Starburst Radio Lines : Galaxies
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordGALACTIC-CENTER REGION ; HUBBLE-SPACE-TELESCOPE ; BODY BARRED MODELS ; A MOLECULAR CLOUD ; CARBON-MONOXIDE ; STAR FORMATION ; INTERSTELLAR-MEDIUM ; ATOMIC CARBON ; PHOTODISSOCIATION REGIONS ; PHYSICAL CONDITIONS
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000088182700014
Citation statistics
Cited Times:137[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8244
Collection分子云与恒星形成研究团组
Affiliation1.Max Planck Inst Radioastron, D-53121 Bonn, Germany
2.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
4.Univ Cologne, Inst Phys & Didakt, D-50931 Cologne, Germany
5.Univ Bonn, Inst Astrophys & Extraterr Forsch, D-53121 Bonn, Germany
6.Univ Cologne, Inst Phys 1, D-50937 Cologne, Germany
7.Univ Arizona, Submillimeter Telescope Observ, Tucson, AZ 85721 USA
8.Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
9.Inst Radioastron Milimetr, Granada 18012, Spain
Recommended Citation
GB/T 7714
Mao, RQ,Henkel, C,Schulz, A,et al. Dense gas in nearby galaxies XIII. CO submillimeter line emission from the starburst galaxy M 82[J]. ASTRONOMY & ASTROPHYSICS,2000,358(2):433-450.
APA Mao, RQ.,Henkel, C.,Schulz, A.,Zielinsky, M.,Mauersberger, R.,...&Gensheimer, P.(2000).Dense gas in nearby galaxies XIII. CO submillimeter line emission from the starburst galaxy M 82.ASTRONOMY & ASTROPHYSICS,358(2),433-450.
MLA Mao, RQ,et al."Dense gas in nearby galaxies XIII. CO submillimeter line emission from the starburst galaxy M 82".ASTRONOMY & ASTROPHYSICS 358.2(2000):433-450.
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