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
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E-Artikel |
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Sprache: |
Englisch |
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1986 |
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3 |
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Springer Online Journal Archives 1860-2002 |
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Übergeordnetes Werk: |
in: Astrophysics and space science - 1968, 118(1986) vom: Jan./Feb., Seite 405-407 |
Übergeordnetes Werk: |
volume:118 ; year:1986 ; month:01/02 ; pages:405-407 ; extent:3 |
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NLEJ193011824 |
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520 | |a 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. | ||
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700 | 1 | |a Ohishi, Masatoshi |4 oth | |
700 | 1 | |a Kaifu, Norio |4 oth | |
700 | 1 | |a Suzuki, Hiroko |4 oth | |
700 | 1 | |a Morimoto, Masaki |4 oth | |
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(DE-627)NLEJ193011824 DE-627 ger DE-627 rakwb eng Excitation of interstellar molecules in the Ori-KL source 1986 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Ohishi, Masatoshi oth Kaifu, Norio oth Suzuki, Hiroko oth Morimoto, Masaki oth in Astrophysics and space science 1968 118(1986) vom: Jan./Feb., Seite 405-407 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:118 year:1986 month:01/02 pages:405-407 extent:3 http://dx.doi.org/10.1007/BF00651157 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 118 1986 1/2 405-407 3 |
spelling |
(DE-627)NLEJ193011824 DE-627 ger DE-627 rakwb eng Excitation of interstellar molecules in the Ori-KL source 1986 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Ohishi, Masatoshi oth Kaifu, Norio oth Suzuki, Hiroko oth Morimoto, Masaki oth in Astrophysics and space science 1968 118(1986) vom: Jan./Feb., Seite 405-407 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:118 year:1986 month:01/02 pages:405-407 extent:3 http://dx.doi.org/10.1007/BF00651157 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 118 1986 1/2 405-407 3 |
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(DE-627)NLEJ193011824 DE-627 ger DE-627 rakwb eng Excitation of interstellar molecules in the Ori-KL source 1986 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Ohishi, Masatoshi oth Kaifu, Norio oth Suzuki, Hiroko oth Morimoto, Masaki oth in Astrophysics and space science 1968 118(1986) vom: Jan./Feb., Seite 405-407 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:118 year:1986 month:01/02 pages:405-407 extent:3 http://dx.doi.org/10.1007/BF00651157 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 118 1986 1/2 405-407 3 |
allfieldsGer |
(DE-627)NLEJ193011824 DE-627 ger DE-627 rakwb eng Excitation of interstellar molecules in the Ori-KL source 1986 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Ohishi, Masatoshi oth Kaifu, Norio oth Suzuki, Hiroko oth Morimoto, Masaki oth in Astrophysics and space science 1968 118(1986) vom: Jan./Feb., Seite 405-407 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:118 year:1986 month:01/02 pages:405-407 extent:3 http://dx.doi.org/10.1007/BF00651157 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 118 1986 1/2 405-407 3 |
allfieldsSound |
(DE-627)NLEJ193011824 DE-627 ger DE-627 rakwb eng Excitation of interstellar molecules in the Ori-KL source 1986 3 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Ohishi, Masatoshi oth Kaifu, Norio oth Suzuki, Hiroko oth Morimoto, Masaki oth in Astrophysics and space science 1968 118(1986) vom: Jan./Feb., Seite 405-407 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:118 year:1986 month:01/02 pages:405-407 extent:3 http://dx.doi.org/10.1007/BF00651157 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 118 1986 1/2 405-407 3 |
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in Astrophysics and space science 118(1986) vom: Jan./Feb., Seite 405-407 volume:118 year:1986 month:01/02 pages:405-407 extent:3 |
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Excitation of interstellar molecules in the Ori-KL source |
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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. |
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. |
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. |
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Excitation of interstellar molecules in the Ori-KL source |
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