The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles
Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite an...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Dorschner, J. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1977 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1977 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 48(1977), 2 vom: Mai, Seite 305-312 |
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| Übergeordnetes Werk: |
volume:48 ; year:1977 ; number:2 ; month:05 ; pages:305-312 |
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|---|
| DOI / URN: |
10.1007/BF00648119 |
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| 245 | 1 | 0 | |a The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles |
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| 520 | |a Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. | ||
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| 700 | 1 | |a Gürtler, J. |4 aut | |
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10.1007/BF00648119 doi (DE-627)OLC2066130206 (DE-He213)BF00648119-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dorschner, J. verfasserin aut The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. Absorption Coefficient Absorption Band Olivine Infrared Spectrum Mass Absorption Friedemann, C. aut Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 48(1977), 2 vom: Mai, Seite 305-312 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:48 year:1977 number:2 month:05 pages:305-312 https://doi.org/10.1007/BF00648119 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 48 1977 2 05 305-312 |
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10.1007/BF00648119 doi (DE-627)OLC2066130206 (DE-He213)BF00648119-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dorschner, J. verfasserin aut The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. Absorption Coefficient Absorption Band Olivine Infrared Spectrum Mass Absorption Friedemann, C. aut Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 48(1977), 2 vom: Mai, Seite 305-312 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:48 year:1977 number:2 month:05 pages:305-312 https://doi.org/10.1007/BF00648119 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 48 1977 2 05 305-312 |
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10.1007/BF00648119 doi (DE-627)OLC2066130206 (DE-He213)BF00648119-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dorschner, J. verfasserin aut The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. Absorption Coefficient Absorption Band Olivine Infrared Spectrum Mass Absorption Friedemann, C. aut Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 48(1977), 2 vom: Mai, Seite 305-312 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:48 year:1977 number:2 month:05 pages:305-312 https://doi.org/10.1007/BF00648119 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 48 1977 2 05 305-312 |
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10.1007/BF00648119 doi (DE-627)OLC2066130206 (DE-He213)BF00648119-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dorschner, J. verfasserin aut The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. Absorption Coefficient Absorption Band Olivine Infrared Spectrum Mass Absorption Friedemann, C. aut Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 48(1977), 2 vom: Mai, Seite 305-312 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:48 year:1977 number:2 month:05 pages:305-312 https://doi.org/10.1007/BF00648119 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 48 1977 2 05 305-312 |
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10.1007/BF00648119 doi (DE-627)OLC2066130206 (DE-He213)BF00648119-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Dorschner, J. verfasserin aut The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. Absorption Coefficient Absorption Band Olivine Infrared Spectrum Mass Absorption Friedemann, C. aut Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 48(1977), 2 vom: Mai, Seite 305-312 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:48 year:1977 number:2 month:05 pages:305-312 https://doi.org/10.1007/BF00648119 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_20 GBV_ILN_21 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_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 48 1977 2 05 305-312 |
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txt |
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305 |
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Dorschner, J. Friedemann, C. Gürtler, J. |
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48 |
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520 530 620 VZ 16,12 ssgn |
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Dorschner, J. |
| doi_str_mv |
10.1007/BF00648119 |
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520 530 620 |
| title_sort |
the 10-micron interstellar absorption band: curves of growth for terrestrial and meteoritic olivine particles |
| title_auth |
The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles |
| abstract |
Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. © D. Reidel Publishing Company 1977 |
| abstractGer |
Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. © D. Reidel Publishing Company 1977 |
| abstract_unstemmed |
Abstract Curves of growth have been determined for the interstellar absorption band at 9.75 μm using infrared spectra of small olivine particles. The mass absorption coefficient was found to depend strongly on the mean radius of the grains. A comparison was made with a sample of Allende meteorite and good agreement was found between the curves of growth for terrestrial and meteoritic olivine. © D. Reidel Publishing Company 1977 |
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2 |
| title_short |
The 10-micron interstellar absorption band: Curves of growth for terrestrial and meteoritic olivine particles |
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