Excitation of interstellar molecules in the Ori-KL source
Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave con...
Ausführliche Beschreibung
Autor*in: |
Ohishi, Masatoshi [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1986 |
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Schlagwörter: |
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Anmerkung: |
© D. Reidel Publishing Company 1986 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 118(1986), 1-2 vom: Jan., Seite 405-407 |
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Übergeordnetes Werk: |
volume:118 ; year:1986 ; number:1-2 ; month:01 ; pages:405-407 |
Links: |
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DOI / URN: |
10.1007/BF00651157 |
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Katalog-ID: |
OLC2066159115 |
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700 | 1 | |a Morimoto, Masaki |4 aut | |
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10.1007/BF00651157 doi (DE-627)OLC2066159115 (DE-He213)BF00651157-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ohishi, Masatoshi verfasserin aut Excitation of interstellar molecules in the Ori-KL source 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. Velocity Component Spectral Line Radial Velocity Line Survey Transition Profile Kaifu, Norio aut Suzuki, Hiroko aut Morimoto, Masaki aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 118(1986), 1-2 vom: Jan., Seite 405-407 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:118 year:1986 number:1-2 month:01 pages:405-407 https://doi.org/10.1007/BF00651157 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 118 1986 1-2 01 405-407 |
spelling |
10.1007/BF00651157 doi (DE-627)OLC2066159115 (DE-He213)BF00651157-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ohishi, Masatoshi verfasserin aut Excitation of interstellar molecules in the Ori-KL source 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. Velocity Component Spectral Line Radial Velocity Line Survey Transition Profile Kaifu, Norio aut Suzuki, Hiroko aut Morimoto, Masaki aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 118(1986), 1-2 vom: Jan., Seite 405-407 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:118 year:1986 number:1-2 month:01 pages:405-407 https://doi.org/10.1007/BF00651157 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 118 1986 1-2 01 405-407 |
allfields_unstemmed |
10.1007/BF00651157 doi (DE-627)OLC2066159115 (DE-He213)BF00651157-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ohishi, Masatoshi verfasserin aut Excitation of interstellar molecules in the Ori-KL source 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. Velocity Component Spectral Line Radial Velocity Line Survey Transition Profile Kaifu, Norio aut Suzuki, Hiroko aut Morimoto, Masaki aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 118(1986), 1-2 vom: Jan., Seite 405-407 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:118 year:1986 number:1-2 month:01 pages:405-407 https://doi.org/10.1007/BF00651157 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 118 1986 1-2 01 405-407 |
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10.1007/BF00651157 doi (DE-627)OLC2066159115 (DE-He213)BF00651157-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ohishi, Masatoshi verfasserin aut Excitation of interstellar molecules in the Ori-KL source 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. Velocity Component Spectral Line Radial Velocity Line Survey Transition Profile Kaifu, Norio aut Suzuki, Hiroko aut Morimoto, Masaki aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 118(1986), 1-2 vom: Jan., Seite 405-407 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:118 year:1986 number:1-2 month:01 pages:405-407 https://doi.org/10.1007/BF00651157 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 118 1986 1-2 01 405-407 |
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10.1007/BF00651157 doi (DE-627)OLC2066159115 (DE-He213)BF00651157-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Ohishi, Masatoshi verfasserin aut Excitation of interstellar molecules in the Ori-KL source 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. Velocity Component Spectral Line Radial Velocity Line Survey Transition Profile Kaifu, Norio aut Suzuki, Hiroko aut Morimoto, Masaki aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 118(1986), 1-2 vom: Jan., Seite 405-407 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:118 year:1986 number:1-2 month:01 pages:405-407 https://doi.org/10.1007/BF00651157 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 118 1986 1-2 01 405-407 |
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abstract |
Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. © D. Reidel Publishing Company 1986 |
abstractGer |
Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. © D. Reidel Publishing Company 1986 |
abstract_unstemmed |
Abstract A molecular spectral line survey of the title source detected 166 molecular lines from 18 interstellar molecules in the frequency ranges of 34.25–50.00, 83.50–84.50, and 86.00–91.50 GHz. For each molecule, gaussian decomposition of the velocity components in the transition profiles gave consistent radial velocity and linewidth. Rotation diagrams were drawn for each velocity component. © D. Reidel Publishing Company 1986 |
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Excitation of interstellar molecules in the Ori-KL source |
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https://doi.org/10.1007/BF00651157 |
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Kaifu, Norio Suzuki, Hiroko Morimoto, Masaki |
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10.1007/BF00651157 |
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